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An extremely bright gamma-ray pulsar in the Large Magellanic Cloud.

Pulsars are rapidly rotating neutron stars that are seen as pulsating sources of radio waves. Some, such as the Crab pulsar, also emit pulses of gamma rays. The Fermi LAT collaboration observed pulsed gamma rays from a pulsar outside our galaxy, the Milky Way. The pulsar, known as PSR J0540-6919, is... Full description

Journal Title: Science (New York N.Y.), November 13, 2015, Vol.350(6262), pp.801-805
Main Author: Ackermann, M
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: E-ISSN: 1095-9203 ; DOI: 10.1126/science.aac7400
Link: http://search.proquest.com/docview/1733194630/?pq-origsite=primo
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title: An extremely bright gamma-ray pulsar in the Large Magellanic Cloud.
format: Article
creator:
  • Ackermann, M
subjects:
  • Gamma Ray Astronomy
  • Pulsars
ispartof: Science (New York, N.Y.), November 13, 2015, Vol.350(6262), pp.801-805
description: Pulsars are rapidly rotating neutron stars that are seen as pulsating sources of radio waves. Some, such as the Crab pulsar, also emit pulses of gamma rays. The Fermi LAT collaboration observed pulsed gamma rays from a pulsar outside our galaxy, the Milky Way. The pulsar, known as PSR J0540-6919, is located in the Large Magellanic Cloud (LMC). This is the most powerful gamma-ray pulsar yet known, with luminosity 20 times that of the Crab. The findings should help to explain how pulsars convert the energy stored in their rotation into detectable electromagnetic emission. Science, this issue p. 801 Pulsars are rapidly spinning, highly magnetized neutron stars, created in the gravitational collapse of massive stars. We report the detection of pulsed giga-electron volt gamma rays from the young pulsar PSR J0540-6919 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This is the first gamma-ray pulsar detected in another galaxy. It has the most luminous pulsed gamma-ray emission...
language: eng
source:
identifier: E-ISSN: 1095-9203 ; DOI: 10.1126/science.aac7400
fulltext: no_fulltext
issn:
  • 10959203
  • 1095-9203
url: Link


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titleAn extremely bright gamma-ray pulsar in the Large Magellanic Cloud.
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ispartofScience (New York, N.Y.), November 13, 2015, Vol.350(6262), pp.801-805
identifierE-ISSN: 1095-9203 ; DOI: 10.1126/science.aac7400
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descriptionPulsars are rapidly rotating neutron stars that are seen as pulsating sources of radio waves. Some, such as the Crab pulsar, also emit pulses of gamma rays. The Fermi LAT collaboration observed pulsed gamma rays from a pulsar outside our galaxy, the Milky Way. The pulsar, known as PSR J0540-6919, is located in the Large Magellanic Cloud (LMC). This is the most powerful gamma-ray pulsar yet known, with luminosity 20 times that of the Crab. The findings should help to explain how pulsars convert the energy stored in their rotation into detectable electromagnetic emission. Science, this issue p. 801 Pulsars are rapidly spinning, highly magnetized neutron stars, created in the gravitational collapse of massive stars. We report the detection of pulsed giga-electron volt gamma rays from the young pulsar PSR J0540-6919 in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. This is the first gamma-ray pulsar detected in another galaxy. It has the most luminous pulsed gamma-ray emission...
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titleAn extremely bright gamma-ray pulsar in the Large Magellanic Cloud.
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103Spandre, G
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113Wood, K S
114Wood, M
115Zampieri, L
atitleAn extremely bright gamma-ray pulsar in the Large Magellanic Cloud.
jtitleScience (New York, N.Y.)
risdate20151113
volume350
issue6262
spage801
epage805
pages801-805
eissn1095-9203
formatjournal
genrearticle
ristypeJOUR
doi10.1126/science.aac7400
urlhttp://search.proquest.com/docview/1733194630/
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
issn00368075
date2015-11-13