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A bright γ-ray flare interpreted as a giant magnetar flare in NGC 253
by
Bozzo, E.
, Starr, R.
, Aptekar, R.
, Rau, A.
, Lysenko, A.
, Barthelmy, S.
, Kozyrev, A.
, Sanin, A.
, Svinkin, D.
, Tsvetkova, A.
, Ubertini, P.
, Ridnaia, A. V.
, Briggs, M. S.
, von Kienlin, A.
, Ferrigno, C.
, Cline, T. L.
, Krimm, H.
, Fellows, C. W.
, Palmer, D. M.
, Golenetskii, S.
, Wilson-Hodge, C.
, Savchenko, V.
, Rodi, J. C.
, Zhang, X.-L.
, Enos, H.
, Frederiks, D.
, Cummings, J.
, Golovin, D.
, Litvak, M.
, Boynton, W.
, Mitrofanov, I.
, Bazzano, A.
, Harshman, K. P.
, Hurley, K.
, Ulanov, M.
, Goldstein, A.
in
639/33/34/4118
/ 639/33/34/4127
/ 639/33/34/864
/ Blackbody
/ Energy
/ Energy flux
/ Flares
/ Fluence
/ Galaxies
/ Gamma rays
/ Gravitation
/ Gravitational waves
/ Gravity
/ Humanities and Social Sciences
/ Light curve
/ Luminosity
/ Magnetars
/ Magnetic fields
/ Morphology
/ multidisciplinary
/ Neutron stars
/ Science
/ Science (multidisciplinary)
2021
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A bright γ-ray flare interpreted as a giant magnetar flare in NGC 253
by
Bozzo, E.
, Starr, R.
, Aptekar, R.
, Rau, A.
, Lysenko, A.
, Barthelmy, S.
, Kozyrev, A.
, Sanin, A.
, Svinkin, D.
, Tsvetkova, A.
, Ubertini, P.
, Ridnaia, A. V.
, Briggs, M. S.
, von Kienlin, A.
, Ferrigno, C.
, Cline, T. L.
, Krimm, H.
, Fellows, C. W.
, Palmer, D. M.
, Golenetskii, S.
, Wilson-Hodge, C.
, Savchenko, V.
, Rodi, J. C.
, Zhang, X.-L.
, Enos, H.
, Frederiks, D.
, Cummings, J.
, Golovin, D.
, Litvak, M.
, Boynton, W.
, Mitrofanov, I.
, Bazzano, A.
, Harshman, K. P.
, Hurley, K.
, Ulanov, M.
, Goldstein, A.
in
639/33/34/4118
/ 639/33/34/4127
/ 639/33/34/864
/ Blackbody
/ Energy
/ Energy flux
/ Flares
/ Fluence
/ Galaxies
/ Gamma rays
/ Gravitation
/ Gravitational waves
/ Gravity
/ Humanities and Social Sciences
/ Light curve
/ Luminosity
/ Magnetars
/ Magnetic fields
/ Morphology
/ multidisciplinary
/ Neutron stars
/ Science
/ Science (multidisciplinary)
2021
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A bright γ-ray flare interpreted as a giant magnetar flare in NGC 253
by
Bozzo, E.
, Starr, R.
, Aptekar, R.
, Rau, A.
, Lysenko, A.
, Barthelmy, S.
, Kozyrev, A.
, Sanin, A.
, Svinkin, D.
, Tsvetkova, A.
, Ubertini, P.
, Ridnaia, A. V.
, Briggs, M. S.
, von Kienlin, A.
, Ferrigno, C.
, Cline, T. L.
, Krimm, H.
, Fellows, C. W.
, Palmer, D. M.
, Golenetskii, S.
, Wilson-Hodge, C.
, Savchenko, V.
, Rodi, J. C.
, Zhang, X.-L.
, Enos, H.
, Frederiks, D.
, Cummings, J.
, Golovin, D.
, Litvak, M.
, Boynton, W.
, Mitrofanov, I.
, Bazzano, A.
, Harshman, K. P.
, Hurley, K.
, Ulanov, M.
, Goldstein, A.
in
639/33/34/4118
/ 639/33/34/4127
/ 639/33/34/864
/ Blackbody
/ Energy
/ Energy flux
/ Flares
/ Fluence
/ Galaxies
/ Gamma rays
/ Gravitation
/ Gravitational waves
/ Gravity
/ Humanities and Social Sciences
/ Light curve
/ Luminosity
/ Magnetars
/ Magnetic fields
/ Morphology
/ multidisciplinary
/ Neutron stars
/ Science
/ Science (multidisciplinary)
2021
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A bright γ-ray flare interpreted as a giant magnetar flare in NGC 253
Journal Article
A bright γ-ray flare interpreted as a giant magnetar flare in NGC 253
2021
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Overview
Soft γ-ray repeaters exhibit bursting emission in hard X-rays and soft γ-rays. During the active phase, they emit random short (milliseconds to several seconds long), hard-X-ray bursts, with peak luminosities
1
of 10
36
to 10
43
erg per second. Occasionally, a giant flare with an energy of around 10
44
to 10
46
erg is emitted
2
. These phenomena are thought to arise from neutron stars with extremely high magnetic fields (10
14
to 10
15
gauss), called magnetars
1
,
3
,
4
. A portion of the second-long initial pulse of a giant flare in some respects mimics short γ-ray bursts
5
,
6
, which have recently been identified as resulting from the merger of two neutron stars accompanied by gravitational-wave emission
7
. Two γ-ray bursts, GRB 051103 and GRB 070201, have been associated with giant flares
2
,
8
–
11
. Here we report observations of the γ-ray burst GRB 200415A, which we localized to a 20-square-arcmin region of the starburst galaxy NGC 253, located about 3.5 million parsecs away. The burst had a sharp, millisecond-scale hard spectrum in the initial pulse, which was followed by steady fading and softening over 0.2 seconds. The energy released (roughly 1.3 × 10
46
erg) is similar to that of the superflare
5
,
12
,
13
from the Galactic soft γ-ray repeater SGR 1806−20 (roughly 2.3 × 10
46
erg). We argue that GRB 200415A is a giant flare from a magnetar in NGC 253.
The γ-ray burst GRB 200415A is probably a giant flare emitted from a magnetar in the nearby starburst galaxy NGC 253.
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