1.8 MeV emission lines from galactic plane region

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1855

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DC Field	Value	Language
dc.contributor.author	Bardoloi, I	-
dc.contributor.author	Duorah, K	-
dc.contributor.author	Duorah, H. L	-
dc.contributor.author	Barua, M. M	-
dc.date.accessioned	2007-10-05T11:55:55Z	-
dc.date.available	2007-10-05T11:55:55Z	-
dc.date.issued	1996	-
dc.identifier.citation	BASI, Vol. 24, No. 4, pp. 749-755	en
dc.identifier.uri	http://hdl.handle.net/2248/1855	-
dc.description.abstract	The COMPTEL telescope aboard the CGRO satellite has revealed highly significant 1.8 MeV emission lines from the Galactic plane region of the Milky Way Galaxy. The observed concentrated emission region may contain a single object or superposition of multiple objects. To explain the observed emission features, an accreting neutron star has been considered as a possible source candidate. During the explosive event in the neutron star, radioactive isotopes of candidate. During the explosive event in the neutron star, radioactive isotopes of 26 AL are produced and ejected into the interstellar matter, wherein 26Alg decays emitting 1.8 MeV gamma-emission lines. The considered candidate should well explain the observed flux of the 1.8 MeV line.	en
dc.format.extent	516849 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..749B	en
dc.subject	1.8 MeV gamma line	en
dc.subject	Neutron star	en
dc.title	1.8 MeV emission lines from galactic plane region	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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