Photometry and Spectroscopy of the GRB 970508 Optical Counterpart

Author:

Castro-Tirado Alberto J.12345,Gorosabel Javier12345,Benı́tez Narciso12345,Wolf Christian12345,Fockenbrock Ralf12345,Martı́nez-González Enrique12345,Kristen Helmuth12345,Broeils Adrick12345,Pedersen Holger12345,Greiner Jochen12345,Costa Enrico12345,Feroci Marco12345,Piro Luigi12345,Frontera Filippo12345,Nicastro Luciano12345,Palazzi Eliana12345,Bartolini Corrado12345,Guarnieri Adriano12345,Masetti Nicola12345,Piccioni Adalberto12345,Mignoli Marco12345,Wold Magrethe12345,Lacy Mark12345,Birkle Kurt12345,Broadhurst Tom12345,Brandt Søren12345,Lund Niels12345

Affiliation:

1. A. J. Castro-Tirado and J. Gorosabel, Laboratorio de Astrofı́sica Espacial y Fı́sica Fundamental, INTA, Madrid, Spain.

2. N. Benı́tez and E. Martı́nez-González, Instituto de Fı́sica de Cantabria, Santander, Spain.

3. C. Wolf, R. Fockenbrock, K. Birkle, Max-Planck-Institut für Astronomie, Heidelberg, Germany.

4. H. Kristen, A. Broeils, M. Wold, Stockholm Observatory, Saltsjobaden, Sweden.

5. H. Pedersen, Copenhagen University Observatory, Copenhagen, Denmark.

Abstract

An optical transient within the error box of the gamma ray burst GRB 970508 was imaged 4 hours after the event. It displayed a strong ultraviolet excess, and reached maximum brightness 2 days later. The optical spectra did not show any emission lines, and no variations on time scales of minutes were observed for 1 hour during the decline phase. According to the fireball and afterglow models, the intensity should rise monotonically before the observed optical maximum, but the data indicate that another physical mechanism may be responsible for the constant phase seen during the first hours after the burst.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference50 articles.

1. For an extensive review of gamma ray burst observations see

2. Fishman G. J., Meegan C. A., Annu. Rev. Astron. Astrophys. 33, 415 (1995).

3. L. Piro L. Scarsi R. C. Butler Proc. SPIE 2517 169 (1995).

4. Frontera F., et al., Astron. Astrophys. Suppl. Ser. 122, 357 (1997).

5. Jager R., et al., ibid. 125, 557 (1997).

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