Interstellar scintillation of the radio source associated with the gamma ray burst of 8 May 1997

Content Provider	Scilit
Author	Smirnova, T. V. Shishov, V. I.
Copyright Year	2000
Description	We show that variability of the radio source associated with the gamma ray burst of May 8, 1997 can be explained by scintillations on interstellar plasma inhomogeneities in the weak regime at 4.86 and 8.46 GHz, and by the refractive component of saturated scintillations at 1.43 GHz. Cosmological distance of this source R ≊ $10^{28}$cm is more preferable. The source has the size about 2μarcsec at frequency 4.86 GHz and the velocity of spreading is about 25μarcsec/year.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/86AD5DC4CF5B238ED151945E1B57D80B/S0252921100060644a.pdf/div-class-title-interstellar-scintillation-of-the-radio-source-associated-with-the-gamma-ray-burst-of-8-may-1997-div.pdf
Ending Page	570
Page Count	2
Starting Page	569
ISSN	02529211
DOI	10.1017/s0252921100060644
Journal	International Astronomical Union Colloquium
Volume Number	177
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2000-01-01
Access Restriction	Open
Subject Keyword	International Astronomical Union Colloquium Astronomy and Astrophysics Source Associated Plasma Inhomogeneities
Content Type	Text
Resource Type	Article