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First observation of ultra-high-energy γ rays from LMC X-4
scientific article published in Nature
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instance of
scholarly article
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title
First observation of ultra-high-energy γ rays from LMC X-4
(English)
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author
Roger W. Clay
series ordinal
2
object named as
R. W. Clay
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author name string
R. J. Protheroe
series ordinal
1
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language of work or name
English
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publication date
May 1985
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published in
Nature
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SIMBAD
volume
315
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stated in
SIMBAD
issue
6016
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page(s)
205–207
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SIMBAD
exact match
https://scigraph.springernature.com/pub.10.1038/315205a0
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cites work
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reference URL
https://api.crossref.org/works/10.1038%2F315205A0
retrieved
21 January 2018
Detection of 2 x l0 l5 to 2 x 10 16 eV gamma-rays from Cygnus X-3
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Crossref
reference URL
https://api.crossref.org/works/10.1038%2F315205A0
retrieved
7 January 2021
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inferred from DOI database lookup
Observation of γ rays >1015 eV from Cygnus X-3
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Crossref
reference URL
https://api.crossref.org/works/10.1038%2F315205A0
retrieved
7 January 2021
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First observations of gamma-rays from Vela X-1 at energies greater than 3x10 15 eV
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Implications of 1016 eV γ rays from Cyg X-3
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Magnetic pair production in Cygnus X-3 and a cut off in the gamma-ray spectrum
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reference URL
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7 January 2021
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Clues from the photonuclear time scale on the nature of particle accelerators in Cygnus X-3 and Vela X-1
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Crossref
reference URL
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retrieved
7 January 2021
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Is Cygnus X-3 a monoenergetic 1017 eV accelerator?
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Cosmic γ rays and cosmic-ray particles
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Search for excess cosmic-ray events from the galactic plane
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Galactic absorption of high-energy gamma-rays from Cygnus X-3
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Crossref
reference URL
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7 January 2021
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Spectroscopic observations and orbit of LMC X-4
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Crossref
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7 January 2021
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Discovery of a 30.5 day periodicity in LMC X-4
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Crossref
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Discovery of 13.5 s X-ray pulsations from LMC X-4 and an orbital determination
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A spectrographic orbit for LMC X-1: another massive X-ray source ?
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A model for 0921-63: a second halo X-ray source
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Observation of Centaurus X-3 by HAKUCHO
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Long-term X-ray observations of Cen X-3, GX 301-2 (4U 1223-62), GX 304-1 (4U 1258-61) and 4U 1145-61
1 reference
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Optical studies of UHURU sources. XI. A probable period for Scorpius X-1 = V818 Scorpii
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4U 1626-67: A prograde spinning X-ray pulsar in A 2500 s binary system
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Crossref
reference URL
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inferred from DOI database lookup
Identifiers
DOI
10.1038/315205A0
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ADS bibcode
1985Natur.315..205P
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SIMBAD
Dimensions Publication ID
1044377191
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