1997NewA....2..449G


Query : 1997NewA....2..449G

1997NewA....2..449G - New Astronomy, 2, 449-460 (1997/November-0)

Radio scintillation of gamma-ray-burst afterglows.

GOODMAN J.

Abstract (from CDS):

Stars twinkle to the eye through atmospheric turbulence, but planets, because of their larger angular size, do not. Similarly, scintillation due to the local interstellar medium will modulate the radio flux of gamma-ray-burst afterglows and may permit indirect measurements of their angular sizes. The amplitude of refractive scintillation is of order ten percent at ten gigahertz unless the source size is much larger than the expected size, of order microarcseconds. Diffractive scintillation is marginally possible, depending sensitively on the source size, observing frequency, and scattering measure of the interstellar medium.

Abstract Copyright: ∼

Journal keyword(s): Gamma rays: bursts - ISM: structure - Scattering - Techniques: interferometric

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
2 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
3 GRB 970111 gB 15 28 15.0 +19 36 18           ~ 140 0
4 4B 960720 gB 17 29.7 +49 20           ~ 54 0

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