Early Observations of the Afterglow of GRB000301c

نویسنده

  • S. G. Bhargavi
چکیده

We report multiband observations of the Optical Transient (OT) associated with GRB000301c carried out between 2–4 March 2000 using the 2.34-m Vainu Bappu Telescope (VBT) at Kavalur, India. When combined with other reported data, the initial decline in the R-band magnitude with log (t − t0), the time since the burst is fit with a slope α1 = -0.70 ± 0.07 which steepens after about 6.0 days to a slope of α2 = -2.44 ± 0.29. This change in slope does not occur smoothly but there is an indication for a bimodal distribution. The available measurements of the evolution of (B–R) color do not show any discernible evolution in the first 12 days. Subject headings: cosmology : observations – gamma rays: bursts.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

On the Probability of Microlensing in GRB Afterglows

The declining lightcurve of the optical afterglow of gamma-ray burst GRB000301C showed rapid variability with one particularly bright feature at about t−t0=3.8 days. This event was interpreted as gravitational microlensing by Garnavich, Loeb & Stanek (2000) and subsequently used to derive constraints on the structure of the GRB optical afterglow. In this paper, we use these structural parameter...

متن کامل

GRB000301C with peculiar afterglow emission

The CCD magnitudes in Johnson V and Cousins R and I photometric passbands are determined for GRB 000301C afterglow starting ∼ 1.5 day after the γ−ray burst. In fact we provide the earliest optical observations for this burst. Light curves of the afterglow emissions are obtained by combining the published data with the present measurements in B,V,R, I, J and K ′ passbands. Flux decay shows a ver...

متن کامل

Letter to the Editor Observations of the soft gamma-ray early afterglow emission from two bright gamma-ray bursts

We present the results of observations of the soft gamma-ray early afterglows with the energy above 100 keV from two bright Gamma-ray bursts detected by the PHEBUS instrument of the GRANAT orbital observatory. We show that the light curves of GRB 910402 and GRB 920723 events present the afterglow emission with fading fluxes. During our observations (∼ 700 s) for these gamma-ray bursts the after...

متن کامل

Observations of the Soft Gamma-Ray early Afterglow emission from Two Bright Gamma-ray Bursts

We present the results of observations of the soft gamma-ray early afterglows with the energy above 100 keV from two bright Gamma-ray bursts detected by the PHEBUS instrument of the GRANAT orbital observatory. We show that the light curves of GRB 910402 and GRB 920723 events present the afterglow emission with fading fluxes. During our observations (∼ 700 s) for these gamma-ray bursts the after...

متن کامل

Gamma-Ray Burst Afterglows with Energy Injection: Homogeneous versus Wind External Media

Assuming an adiabatic evolution of a gamma-ray burst (hereafter GRB) fireball interacting with an external medium, we calculate the hydrodynamics of the fireball with energy injection from a strongly magnetic millisecond pulsar through magnetic dipole radiation, and we obtain the light curve of the optical afterglow from the fireball by synchrotron radiation. Results are given both for a homoge...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2000