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A population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope

Pulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to mi... Full description

Journal Title: Science (New York N.Y.), 14 August 2009, Vol.325(5942), pp.848-52
Main Author: Abdo, A A
Other Authors: Ackermann, M , Ajello, M , Atwood, W B , Axelsson, M , Baldini, L , Ballet, J , Barbiellini, G , Baring, M G , Bastieri, D , Baughman, B M , Bechtol, K , Bellazzini, R , Berenji, B , Bignami, G F , Blandford, R D , Bloom, E D , Bonamente, E , Borgland, A W , Bregeon, J , Brez, A , Brigida, M , Bruel, P , Burnett, T H , Caliandro, G A , Cameron, R A , Camilo, F , Caraveo, P A , Carlson, P , Casandjian, J M , Cecchi, C , Celik, O , Charles, E , Chekhtman, A , Cheung, C C , Chiang, J , Ciprini, S , Claus, R , Cognard, I , Cohen-Tanugi, J , Cominsky, L R , Conrad, J , Corbet, R , Cutini, S , Dermer, C D , Desvignes, G , De Angelis, A , De Luca, A , De Palma, F , Digel, S W , Dormody, M , Do Couto E Silva, E , Drell, P S , Dubois, R , Dumora, D , Edmonds, Y , Farnier, C , Favuzzi, C , Fegan, S J , Focke, W B , Frailis, M , Freire, P C C , Fukazawa, Y , Funk, S , Fusco, P , Gargano, F , Gasparrini, D , Gehrels, N , Germani, S , Giebels, B , Giglietto, N , Giordano, F , Glanzman, T , Godfrey, G , Grenier, I A , Grondin, M H , Grove, J E , Guillemot, L , Guiriec, S , Hanabata, Y , Harding, A K , Hayashida, M , Hays, E , Hobbs, G , Hughes, R E , Jóhannesson, G , Johnson, A S , Johnson, R P , Johnson, T J , Johnson, W N , Johnston, S , Kamae, T , Katagiri, H , Kataoka, J , Kawai, N , Kerr, M , Knödlseder, J , Kocian, M L , Kramer, M , Kuss, M , Lande, J , Latronico, L , Lemoine-Goumard, M , Longo, F , Loparco, F , Lott, B , Lovellette, M N , Lubrano, P , Madejski, G M , Makeev, A , Manchester, R N , Marelli, M , Mazziotta, M N , Mcconville, W , Mcenery, J E , Mclaughlin, M A , Meurer, C , Michelson, P F , Mitthumsiri, W , Mizuno, T , Moiseev, A A , Monte, C , Monzani, M E , Morselli, A , Moskalenko, I V , Murgia, S , Nolan, P L , Norris, J P , Nuss, E , Ohsugi, T , Omodei, N , Orlando, E , Ormes, J F , Paneque, D , Panetta, J H , Parent, D , Pelassa, V , Pepe, M , Pesce-Rollins, M , Piron, F , Porter, T A , Rainò, S , Rando, R , Ransom, S M , Ray, P S , Razzano, M , Rea, N , Reimer, A , Reimer, O , Reposeur, T , Ritz, S , Rochester, L S , Rodriguez, A Y , Romani, R W , Roth, M , Ryde, F , Sadrozinski, H F W , Sanchez, D , Sander, A , Saz Parkinson, P M , Scargle, J D , Schalk, T L , Sgrò, C , Siskind, E J , Smith, D A , Smith, P D , Spandre, G , Spinelli, P , Stappers, B W , Starck, J L , Striani, E , Strickman, M S , Suson, D J , Tajima, H , Takahashi, H , Tanaka, T , Thayer, J B , Thayer, J G , Theureau, G , Thompson, D J , Thorsett, S E , Tibaldo, L , Torres, D F , Tosti, G , Tramacere, A , Uchiyama, Y , Usher, T L , Van Etten, A , Vasileiou, V , Venter, C , Vilchez, N , Vitale, V , Waite, A P , Wallace, E , Wang, P , Watters, K , Webb, N , Weltevrede, P , Winer, B L , Wood, K S , Ylinen, T , Ziegler, M
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; PMID: 19574349 Version:1 ; DOI: 10.1126/science.1176113
Link: http://pubmed.gov/19574349
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recordid: medline19574349
title: A population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope
format: Article
creator:
  • Abdo, A A
  • Ackermann, M
  • Ajello, M
  • Atwood, W B
  • Axelsson, M
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Baring, M G
  • Bastieri, D
  • Baughman, B M
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Bignami, G F
  • Blandford, R D
  • Bloom, E D
  • Bonamente, E
  • Borgland, A W
  • Bregeon, J
  • Brez, A
  • Brigida, M
  • Bruel, P
  • Burnett, T H
  • Caliandro, G A
  • Cameron, R A
  • Camilo, F
  • Caraveo, P A
  • Carlson, P
  • Casandjian, J M
  • Cecchi, C
  • Celik, O
  • Charles, E
  • Chekhtman, A
  • Cheung, C C
  • Chiang, J
  • Ciprini, S
  • Claus, R
  • Cognard, I
  • Cohen-Tanugi, J
  • Cominsky, L R
  • Conrad, J
  • Corbet, R
  • Cutini, S
  • Dermer, C D
  • Desvignes, G
  • De Angelis, A
  • De Luca, A
  • De Palma, F
  • Digel, S W
  • Dormody, M
  • Do Couto E Silva, E
  • Drell, P S
  • Dubois, R
  • Dumora, D
  • Edmonds, Y
  • Farnier, C
  • Favuzzi, C
  • Fegan, S J
  • Focke, W B
  • Frailis, M
  • Freire, P C C
  • Fukazawa, Y
  • Funk, S
  • Fusco, P
  • Gargano, F
  • Gasparrini, D
  • Gehrels, N
  • Germani, S
  • Giebels, B
  • Giglietto, N
  • Giordano, F
  • Glanzman, T
  • Godfrey, G
  • Grenier, I A
  • Grondin, M H
  • Grove, J E
  • Guillemot, L
  • Guiriec, S
  • Hanabata, Y
  • Harding, A K
  • Hayashida, M
  • Hays, E
  • Hobbs, G
  • Hughes, R E
  • Jóhannesson, G
  • Johnson, A S
  • Johnson, R P
  • Johnson, T J
  • Johnson, W N
  • Johnston, S
  • Kamae, T
  • Katagiri, H
  • Kataoka, J
  • Kawai, N
  • Kerr, M
  • Knödlseder, J
  • Kocian, M L
  • Kramer, M
  • Kuss, M
  • Lande, J
  • Latronico, L
  • Lemoine-Goumard, M
  • Longo, F
  • Loparco, F
  • Lott, B
  • Lovellette, M N
  • Lubrano, P
  • Madejski, G M
  • Makeev, A
  • Manchester, R N
  • Marelli, M
  • Mazziotta, M N
  • Mcconville, W
  • Mcenery, J E
  • Mclaughlin, M A
  • Meurer, C
  • Michelson, P F
  • Mitthumsiri, W
  • Mizuno, T
  • Moiseev, A A
  • Monte, C
  • Monzani, M E
  • Morselli, A
  • Moskalenko, I V
  • Murgia, S
  • Nolan, P L
  • Norris, J P
  • Nuss, E
  • Ohsugi, T
  • Omodei, N
  • Orlando, E
  • Ormes, J F
  • Paneque, D
  • Panetta, J H
  • Parent, D
  • Pelassa, V
  • Pepe, M
  • Pesce-Rollins, M
  • Piron, F
  • Porter, T A
  • Rainò, S
  • Rando, R
  • Ransom, S M
  • Ray, P S
  • Razzano, M
  • Rea, N
  • Reimer, A
  • Reimer, O
  • Reposeur, T
  • Ritz, S
  • Rochester, L S
  • Rodriguez, A Y
  • Romani, R W
  • Roth, M
  • Ryde, F
  • Sadrozinski, H F W
  • Sanchez, D
  • Sander, A
  • Saz Parkinson, P M
  • Scargle, J D
  • Schalk, T L
  • Sgrò, C
  • Siskind, E J
  • Smith, D A
  • Smith, P D
  • Spandre, G
  • Spinelli, P
  • Stappers, B W
  • Starck, J L
  • Striani, E
  • Strickman, M S
  • Suson, D J
  • Tajima, H
  • Takahashi, H
  • Tanaka, T
  • Thayer, J B
  • Thayer, J G
  • Theureau, G
  • Thompson, D J
  • Thorsett, S E
  • Tibaldo, L
  • Torres, D F
  • Tosti, G
  • Tramacere, A
  • Uchiyama, Y
  • Usher, T L
  • Van Etten, A
  • Vasileiou, V
  • Venter, C
  • Vilchez, N
  • Vitale, V
  • Waite, A P
  • Wallace, E
  • Wang, P
  • Watters, K
  • Webb, N
  • Weltevrede, P
  • Winer, B L
  • Wood, K S
  • Ylinen, T
  • Ziegler, M
subjects:
  • Space Telescopes
  • Pulsars
  • Gamma Ray Astronomy
ispartof: Science (New York, N.Y.), 14 August 2009, Vol.325(5942), pp.848-52
description: Pulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.
language: eng
source:
identifier: E-ISSN: 1095-9203 ; PMID: 19574349 Version:1 ; DOI: 10.1126/science.1176113
fulltext: fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleA population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope
creatorAbdo, A A ; Ackermann, M ; Ajello, M ; Atwood, W B ; Axelsson, M ; Baldini, L ; Ballet, J ; Barbiellini, G ; Baring, M G ; Bastieri, D ; Baughman, B M ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bignami, G F ; Blandford, R D ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Caliandro, G A ; Cameron, R A ; Camilo, F ; Caraveo, P A ; Carlson, P ; Casandjian, J M ; Cecchi, C ; Celik, O ; Charles, E ; Chekhtman, A ; Cheung, C C ; Chiang, J ; Ciprini, S ; Claus, R ; Cognard, I ; Cohen-Tanugi, J ; Cominsky, L R ; Conrad, J ; Corbet, R ; Cutini, S ; Dermer, C D ; Desvignes, G ; De Angelis, A ; De Luca, A ; De Palma, F ; Digel, S W ; Dormody, M ; Do Couto E Silva, E ; Drell, P S ; Dubois, R ; Dumora, D ; Edmonds, Y ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Focke, W B ; Frailis, M ; Freire, P C C ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giebels, B ; Giglietto, N ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grondin, M H ; Grove, J E ; Guillemot, L ; Guiriec, S ; Hanabata, Y ; Harding, A K ; Hayashida, M ; Hays, E ; Hobbs, G ; Hughes, R E ; Jóhannesson, G ; Johnson, A S ; Johnson, R P ; Johnson, T J ; Johnson, W N ; Johnston, S ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kocian, M L ; Kramer, M ; Kuss, M ; Lande, J ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Madejski, G M ; Makeev, A ; Manchester, R N ; Marelli, M ; Mazziotta, M N ; Mcconville, W ; Mcenery, J E ; Mclaughlin, M A ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Moiseev, A A ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Paneque, D ; Panetta, J H ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Piron, F ; Porter, T A ; Rainò, S ; Rando, R ; Ransom, S M ; Ray, P S ; Razzano, M ; Rea, N ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Rochester, L S ; Rodriguez, A Y ; Romani, R W ; Roth, M ; Ryde, F ; Sadrozinski, H F W ; Sanchez, D ; Sander, A ; Saz Parkinson, P M ; Scargle, J D ; Schalk, T L ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Stappers, B W ; Starck, J L ; Striani, E ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Tanaka, T ; Thayer, J B ; Thayer, J G ; Theureau, G ; Thompson, D J ; Thorsett, S E ; Tibaldo, L ; Torres, D F ; Tosti, G ; Tramacere, A ; Uchiyama, Y ; Usher, T L ; Van Etten, A ; Vasileiou, V ; Venter, C ; Vilchez, N ; Vitale, V ; Waite, A P ; Wallace, E ; Wang, P ; Watters, K ; Webb, N ; Weltevrede, P ; Winer, B L ; Wood, K S ; Ylinen, T ; Ziegler, M
ispartofScience (New York, N.Y.), 14 August 2009, Vol.325(5942), pp.848-52
identifier
descriptionPulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.
languageeng
source
subjectSpace Telescopes ; Pulsars ; Gamma Ray Astronomy;
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0Abdo, A A
1Ackermann, M
2Ajello, M
3Atwood, W B
4Axelsson, M
5Baldini, L
6Ballet, J
7Barbiellini, G
8Baring, M G
9Bastieri, D
10Baughman, B M
11Bechtol, K
12Bellazzini, R
13Berenji, B
14Bignami, G F
15Blandford, R D
16Bloom, E D
17Bonamente, E
18Borgland, A W
19Bregeon, J
20Brez, A
21Brigida, M
22Bruel, P
23Burnett, T H
24Caliandro, G A
25Cameron, R A
26Camilo, F
27Caraveo, P A
28Carlson, P
29Casandjian, J M
30Cecchi, C
31Celik, O
32Charles, E
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cognard, I
39Cohen-Tanugi, J
40Cominsky, L R
41Conrad, J
42Corbet, R
43Cutini, S
44Dermer, C D
45Desvignes, G
46de Angelis, A
47de Luca, A
48de Palma, F
49Digel, S W
50Dormody, M
51do Couto e Silva, E
52Drell, P S
53Dubois, R
54Dumora, D
55Edmonds, Y
56Farnier, C
57Favuzzi, C
58Fegan, S J
59Focke, W B
60Frailis, M
61Freire, P C C
62Fukazawa, Y
63Funk, S
64Fusco, P
65Gargano, F
66Gasparrini, D
67Gehrels, N
68Germani, S
69Giebels, B
70Giglietto, N
71Giordano, F
72Glanzman, T
73Godfrey, G
74Grenier, I A
75Grondin, M H
76Grove, J E
77Guillemot, L
78Guiriec, S
79Hanabata, Y
80Harding, A K
81Hayashida, M
82Hays, E
83Hobbs, G
84Hughes, R E
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Johnston, S
91Kamae, T
92Katagiri, H
93Kataoka, J
94Kawai, N
95Kerr, M
96Knödlseder, J
97Kocian, M L
98Kramer, M
99Kuss, M
100...
titleA population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope
descriptionPulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.
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titleA population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope
authorAbdo, A A ; Ackermann, M ; Ajello, M ; Atwood, W B ; Axelsson, M ; Baldini, L ; Ballet, J ; Barbiellini, G ; Baring, M G ; Bastieri, D ; Baughman, B M ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bignami, G F ; Blandford, R D ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Caliandro, G A ; Cameron, R A ; Camilo, F ; Caraveo, P A ; Carlson, P ; Casandjian, J M ; Cecchi, C ; Celik, O ; Charles, E ; Chekhtman, A ; Cheung, C C ; Chiang, J ; Ciprini, S ; Claus, R ; Cognard, I ; Cohen-Tanugi, J ; Cominsky, L R ; Conrad, J ; Corbet, R ; Cutini, S ; Dermer, C D ; Desvignes, G ; De Angelis, A ; De Luca, A ; De Palma, F ; Digel, S W ; Dormody, M ; Do Couto E Silva, E ; Drell, P S ; Dubois, R ; Dumora, D ; Edmonds, Y ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Focke, W B ; Frailis, M ; Freire, P C C ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giebels, B ; Giglietto, N ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grondin, M H ; Grove, J E ; Guillemot, L ; Guiriec, S ; Hanabata, Y ; Harding, A K ; Hayashida, M ; Hays, E ; Hobbs, G ; Hughes, R E ; Jóhannesson, G ; Johnson, A S ; Johnson, R P ; Johnson, T J ; Johnson, W N ; Johnston, S ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kocian, M L ; Kramer, M ; Kuss, M ; Lande, J ; Latronico, L ; Lemoine-Goumard, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Madejski, G M ; Makeev, A ; Manchester, R N ; Marelli, M ; Mazziotta, M N ; Mcconville, W ; Mcenery, J E ; Mclaughlin, M A ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Moiseev, A A ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Paneque, D ; Panetta, J H ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Piron, F ; Porter, T A ; Rainò, S ; Rando, R ; Ransom, S M ; Ray, P S ; Razzano, M ; Rea, N ; Reimer, A ; Reimer, O ; Reposeur, T ; Ritz, S ; Rochester, L S ; Rodriguez, A Y ; Romani, R W ; Roth, M ; Ryde, F ; Sadrozinski, H F W ; Sanchez, D ; Sander, A ; Saz Parkinson, P M ; Scargle, J D ; Schalk, T L ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Stappers, B W ; Starck, J L ; Striani, E ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Tanaka, T ; Thayer, J B ; Thayer, J G ; Theureau, G ; Thompson, D J ; Thorsett, S E ; Tibaldo, L ; Torres, D F ; Tosti, G ; Tramacere, A ; Uchiyama, Y ; Usher, T L ; Van Etten, A ; Vasileiou, V ; Venter, C ; Vilchez, N ; Vitale, V ; Waite, A P ; Wallace, E ; Wang, P ; Watters, K ; Webb, N ; Weltevrede, P ; Winer, B L ; Wood, K S ; Ylinen, T ; Ziegler, M
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0Abdo, A A
1Ackermann, M
2Ajello, M
3Atwood, W B
4Axelsson, M
5Baldini, L
6Ballet, J
7Barbiellini, G
8Baring, M G
9Bastieri, D
10Baughman, B M
11Bechtol, K
12Bellazzini, R
13Berenji, B
14Bignami, G F
15Blandford, R D
16Bloom, E D
17Bonamente, E
18Borgland, A W
19Bregeon, J
20Brez, A
21Brigida, M
22Bruel, P
23Burnett, T H
24Caliandro, G A
25Cameron, R A
26Camilo, F
27Caraveo, P A
28Carlson, P
29Casandjian, J M
30Cecchi, C
31Celik, O
32Charles, E
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cognard, I
39Cohen-Tanugi, J
40Cominsky, L R
41Conrad, J
42Corbet, R
43Cutini, S
44Dermer, C D
45Desvignes, G
46De Angelis, A
47De Luca, A
48De Palma, F
49Digel, S W
50Dormody, M
51Do Couto E Silva, E
52Drell, P S
53Dubois, R
54Dumora, D
55Edmonds, Y
56Farnier, C
57Favuzzi, C
58Fegan, S J
59Focke, W B
60Frailis, M
61Freire, P C C
62Fukazawa, Y
63Funk, S
64Fusco, P
65Gargano, F
66Gasparrini, D
67Gehrels, N
68Germani, S
69Giebels, B
70Giglietto, N
71Giordano, F
72Glanzman, T
73Godfrey, G
74Grenier, I A
75Grondin, M H
76Grove, J E
77Guillemot, L
78Guiriec, S
79Hanabata, Y
80Harding, A K
81Hayashida, M
82Hays, E
83Hobbs, G
84Hughes, R E
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Johnston, S
91Kamae, T
92Katagiri, H
93Kataoka, J
94Kawai, N
95Kerr, M
96Knödlseder, J
97Kocian, M L
98Kramer, M
99Kuss, M
100...
jtitleScience (New York, N.Y.)
toplevelpeer_reviewed
delivery
delcategoryRemote Search Resource
fulltextfulltext
addata
aulast
0Abdo
1Ackermann
2Ajello
3Atwood
4Axelsson
5Baldini
6Ballet
7Barbiellini
8Baring
9Bastieri
10Baughman
11Bechtol
12Bellazzini
13Berenji
14Bignami
15Blandford
16Bloom
17Bonamente
18Borgland
19Bregeon
20Brez
21Brigida
22Bruel
23Burnett
24Caliandro
25Cameron
26Camilo
27Caraveo
28Carlson
29Casandjian
30Cecchi
31Celik
32Charles
33Chekhtman
34Cheung
35Chiang
36Ciprini
37Claus
38Cognard
39Cohen-Tanugi
40Cominsky
41Conrad
42Corbet
43Cutini
44Dermer
45Desvignes
46de Angelis
47de Luca
48de Palma
49Digel
50Dormody
51Do Couto E Silva
52Drell
53Dubois
54Dumora
55Edmonds
56Farnier
57Favuzzi
58Fegan
59Focke
60Frailis
61Freire
62Fukazawa
63Funk
64Fusco
65Gargano
66Gasparrini
67Gehrels
68Germani
69Giebels
70Giglietto
71Giordano
72Glanzman
73Godfrey
74Grenier
75Grondin
76Grove
77Guillemot
78Guiriec
79Hanabata
80Harding
81Hayashida
82Hays
83Hobbs
84Hughes
85Jóhannesson
86Johnson
87Johnston
88Kamae
89Katagiri
90Kataoka
91Kawai
92Kerr
93Knödlseder
94Kocian
95Kramer
96Kuss
97Lande
98Latronico
99Lemoine-Goumard
100...
aufirst
0A A
1M
2W B
3L
4J
5G
6M G
7D
8B M
9K
10R
11B
12G F
13R D
14E D
15E
16A W
17A
18P
19T H
20G A
21R A
22F
23P A
24J M
25C
26O
27C C
28S
29I
30L R
31C D
32S W
33P S
34Y
35S J
36P C C
37N
38T
39I A
40M H
41J E
42A K
43R E
44A S
45R P
46T J
47W N
48H
49M L
50M N
51G M
52R N
53W
54M A
55P F
56M E
57I V
58P L
59J P
60J F
61J H
62V
63T A
64S M
65L S
66A Y
67R W
68H F W
69P M
70J D
71T L
72E J
73D A
74P D
75B W
76J L
77M S
78D J
79J B
80J G
81S E
82D F
83A P
84B L
85K S
au
0Abdo, A A
1Ackermann, M
2Ajello, M
3Atwood, W B
4Axelsson, M
5Baldini, L
6Ballet, J
7Barbiellini, G
8Baring, M G
9Bastieri, D
10Baughman, B M
11Bechtol, K
12Bellazzini, R
13Berenji, B
14Bignami, G F
15Blandford, R D
16Bloom, E D
17Bonamente, E
18Borgland, A W
19Bregeon, J
20Brez, A
21Brigida, M
22Bruel, P
23Burnett, T H
24Caliandro, G A
25Cameron, R A
26Camilo, F
27Caraveo, P A
28Carlson, P
29Casandjian, J M
30Cecchi, C
31Celik, O
32Charles, E
33Chekhtman, A
34Cheung, C C
35Chiang, J
36Ciprini, S
37Claus, R
38Cognard, I
39Cohen-Tanugi, J
40Cominsky, L R
41Conrad, J
42Corbet, R
43Cutini, S
44Dermer, C D
45Desvignes, G
46de Angelis, A
47de Luca, A
48de Palma, F
49Digel, S W
50Dormody, M
51Do Couto E Silva, E
52Drell, P S
53Dubois, R
54Dumora, D
55Edmonds, Y
56Farnier, C
57Favuzzi, C
58Fegan, S J
59Focke, W B
60Frailis, M
61Freire, P C C
62Fukazawa, Y
63Funk, S
64Fusco, P
65Gargano, F
66Gasparrini, D
67Gehrels, N
68Germani, S
69Giebels, B
70Giglietto, N
71Giordano, F
72Glanzman, T
73Godfrey, G
74Grenier, I A
75Grondin, M H
76Grove, J E
77Guillemot, L
78Guiriec, S
79Hanabata, Y
80Harding, A K
81Hayashida, M
82Hays, E
83Hobbs, G
84Hughes, R E
85Jóhannesson, G
86Johnson, A S
87Johnson, R P
88Johnson, T J
89Johnson, W N
90Johnston, S
91Kamae, T
92Katagiri, H
93Kataoka, J
94Kawai, N
95Kerr, M
96Knödlseder, J
97Kocian, M L
98Kramer, M
99Kuss, M
100...
atitleA population of gamma-ray millisecond pulsars seen with the Fermi Large Area Telescope
jtitleScience (New York, N.Y.)
risdate20090814
volume325
issue5942
spage848
pages848-852
eissn1095-9203
formatjournal
genrearticle
ristypeJOUR
abstractPulsars are born with subsecond spin periods and slow by electromagnetic braking for several tens of millions of years, when detectable radiation ceases. A second life can occur for neutron stars in binary systems. They can acquire mass and angular momentum from their companions, to be spun up to millisecond periods and begin radiating again. We searched Fermi Large Area Telescope data for pulsations from all known millisecond pulsars (MSPs) outside of globular clusters, using rotation parameters from radio telescopes. Strong gamma-ray pulsations were detected for eight MSPs. The gamma-ray pulse profiles and spectral properties resemble those of young gamma-ray pulsars. The basic emission mechanism seems to be the same for MSPs and young pulsars, with the emission originating in regions far from the neutron star surface.
doi10.1126/science.1176113
pmid19574349
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
issn00368075
oafree_for_read
date2009-08-14