If at cosmological distances, a small fraction of gamma-ray bursts should be multiply imaged by intervening galaxies or clusters, resulting in the appearance of two very similar bursts from the same location with a relative time delay of hours to a year. We show that microlensing by individual stars in the lensing galaxy can smear out the light curves of the multiply imaged bursts on millisecond time scales. Therefore, in deciding whether two bursts are similar enough to qualify as multiple images, one must look at time scales longer than a few tens of milliseconds, since shorter time scales are possibly rendered dissimilar by microlensing. Key words: gamma-ray bursts -- gravitational lensing. 1 INTRODUCTION After more than two decades of...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
Open Access.All quasars vary in their optical flux on a timescale of years, and it has been proposed...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
If they are located at cosmological distances, a small fraction of gamma-ray bursts should be multip...
The microlensing effect has developed into a powerful technique for a diverse range of applications ...
The microlensing interpretation of the optical afterglow of GRB 000301C seems naively surprising, si...
The afterglow of a cosmological Gamma-Ray Burst (GRB) should appear on the sky as a narrow emission ...
The optical afterglow of gamma-ray burst (GRB) 000301C exhibited a signiÐcant, short timescale devi-...
In microlensing of a Galactic star by a brown dwarf or other compact object, the amplified image rea...
Gamma-ray bursts (GRBs) vary more rapidly than any other known cosmological phenomena. The lower lim...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
The photometric history of the events related to Gamma-Ray Bursts can be studied from the very begin...
The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has b...
With upcoming (continuum) surveys of high-resolution radio telescopes, detection rates of fast radio...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
Open Access.All quasars vary in their optical flux on a timescale of years, and it has been proposed...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...
If they are located at cosmological distances, a small fraction of gamma-ray bursts should be multip...
The microlensing effect has developed into a powerful technique for a diverse range of applications ...
The microlensing interpretation of the optical afterglow of GRB 000301C seems naively surprising, si...
The afterglow of a cosmological Gamma-Ray Burst (GRB) should appear on the sky as a narrow emission ...
The optical afterglow of gamma-ray burst (GRB) 000301C exhibited a signiÐcant, short timescale devi-...
In microlensing of a Galactic star by a brown dwarf or other compact object, the amplified image rea...
Gamma-ray bursts (GRBs) vary more rapidly than any other known cosmological phenomena. The lower lim...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
If the objects responsible for gravitational microlensing (ML) of Galactic-bulge stars are faint dwa...
The photometric history of the events related to Gamma-Ray Bursts can be studied from the very begin...
The recent discovery that faint gamma-ray bursts are stretched in time relative to bright ones has b...
With upcoming (continuum) surveys of high-resolution radio telescopes, detection rates of fast radio...
The phenomena of gravitational microlensing are described, and predictions are made about its possib...
Open Access.All quasars vary in their optical flux on a timescale of years, and it has been proposed...
In the next future, astrometric microlensing will offer a new channel for investigating the nature o...