NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Cyclotron resonant scattering in gamma-ray bursts - Line strengths and signature of neutron star rotationWe explain the relative line strengths in gamma-ray bursts in terms of cyclotron resonant scattering. We describe the line signature of neutron star rotation and discuss the possibility that variations seen in the strengths and widths of the lines in GB780325 and GB870303 are due to rotation.
Document ID
19930036255
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Lamb, D. Q. (Chicago Univ. IL, United States)
Wang, J. C. L. (Chicago Univ. IL; Canadian Inst. for Theoretical Astrophysics, Toronto, Canada)
Wasserman, I. (Cornell Univ. Ithaca, NY, United States)
Date Acquired
August 15, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Gamma-ray bursts - Observations, analyses and theories (A93-20206 06-90)
Publisher: Cambridge University Press
Subject Category
Astrophysics
Accession Number
93A20252
Funding Number(s)
CONTRACT_GRANT: NAG5-1177
CONTRACT_GRANT: NAGW-1284
CONTRACT_GRANT: NAGW-666
CONTRACT_GRANT: NSF AST-89-13112
CONTRACT_GRANT: NAGW-830
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.

Related Records

There are no records associated with this record.
No Preview Available