Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-03-15
Astrophys.J. 534 (2000) 248-257
Astronomy and Astrophysics
Astrophysics
25 pages + 6 figures, submitted to ApJ; Revised September 27, 1999 with additonal table, new versions of two figures, and revi
Scientific paper
10.1086/308725
We suggest a connection between the pulse paradigm at gamma-ray energies and the recently demonstrated luminosity distribution in gamma-ray bursts: the spectral evolution timescale of pulse structures is anticorrelated with peak luminosity, and with quantities which might be expected to reflect the bulk relativistic Lorentz factor, such as spectral hardness ratio. We establish this relationship in two important burst samples using the cross-correlation lags between low (25-50 keV) and high (100-300 keV and > 300 keV) energy bands. For a set of seven bursts (six with redshifts) observed by CGRO/BATSE and BeppoSAX which also have optical or radio counterparts, the gamma/X peak flux ratios and peak luminosities are anti-correlated with spectral lag. For the 174 brightest BATSE bursts with durations longer than 2 s and significant emission above 300 keV, a similar anti-correlation is evident between gamma-ray hardness ratio or peak flux, and spectral lag. For the six bursts with redshifts, the connection between peak luminosity and spectral lag is well-fitted by a power-law. GRB 980425 (if associated with SN 1998bw) would appear to extend this trend qualitatively, but with a lag of ~ 4-5 s and luminosity of ~ 1.3x10^47 ergs s^-1, it falls below the power-law relationship by a factor of ~ 460. As noted previously by Band, most lags are concentrated on the short end of the lag distribution, near 100 ms, suggesting that the GRB luminosity distribution is peaked on its high end, e.g. N(L) proportional to L^beta, with positive beta.
Bonnell Jerry T.
Marani Gabriela Fabiana
Norris Jay P.
No associations
LandOfFree
Connection Between Energy-dependent Lags And Peak Luminosity In Gamma-ray Bursts does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Connection Between Energy-dependent Lags And Peak Luminosity In Gamma-ray Bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Connection Between Energy-dependent Lags And Peak Luminosity In Gamma-ray Bursts will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-538188