Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Science 26 March 1999:
Vol. 283. no. 5410, pp. 2069 - 2073
DOI: 10.1126/science.283.5410.2069

Reports

Decay of the GRB 990123 Optical Afterglow: Implications for the Fireball Model

Alberto J. Castro-Tirado, 15* María Rosa Zapatero-Osorio, 2 Nicola Caon, 2 Luz Marina Cairós, 2 Jens Hjorth, 3 Holger Pedersen, 3 Michael I. Andersen, 4 Javier Gorosabel, 5 Corrado Bartolini, 6 Adriano Guarnieri, 6 Adalberto Piccioni, 6 Filippo Frontera, 78 Nicola Masetti, 8 Eliana Palazzi, 8 Elena Pian, 8 Jochen Greiner, 9 Renè Hudec, 10 Ram Sagar, 11 Anil K. Pandey, 11 Vinay Mohan, 11 Ramakant K. S. Yadav, 11 Nilakshi, 11 Gunnlaugur Björnsson, 12 Páll Jakobsson, 12 Ingunn Burud, 13 Frederic Courbin, 13 Gaetano Valentini, 14 Anna Piersimoni, 14 Jesús Aceituno, 15 Luz María Montoya, 15 Santos Pedraz, 15 Roland Gredel, 15 Charles F. Claver, 16 Travis A. Rector, 16 James E. Rhoads, 16 Fabian Walter, 17 Jürgen Ott, 18 Hans Hippelein, 19 Victor Sánchez-Béjar, 2 Carlos Gutiérrez, 2 Alejandro Oscoz, 2 Jin Zhu, 20 Jiansheng Chen, 20 Haotong Zhang, 20 Jianyan Wei, 20 Aiying Zhou, 20 Sergei Guziy, 21 Aleksei Shlyapnikov, 22 John Heise, 23 Enrico Costa, 24 Marco Feroci, 24 Luigi Piro 24

Broad-band (ultraviolet to near-infrared) observations of the intense gamma ray burst GRB 990123 started ~8.5 hours after the event and continued until 18 February 1999. When combined with other data, in particular from the Robotic Telescope and Transient Source Experiment (ROTSE) and the Hubble Space Telescope (HST), evidence emerges for a smoothly declining light curve, suggesting some color dependence that could be related to a cooling break passing the ultraviolet-optical band at about 1 day after the high-energy event. The steeper decline rate seen after 1.5 to 2 days may be evidence for a collimated jet pointing toward the observer.

1 Instituto de Astrofísica de Andalucía, IAA-CSIC, Granada, Spain.
2 Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain.
3 Astronomical Observatory, University of Copenhagen, Copenhagen, Denmark.
4 Nordic Optical Telescope, La Palma, Tenerife, Spain.
5 Laboratorio de Astrofísica Espacial y Física Fundamental, INTA, Madrid, Spain.
6 Dipartimento di Astronomia, Università di Bologna, Bologna, Italy.
7 Dipartimento di Fisica, Università di Ferrara, Ferrara, Italy.
8 Istituto Tecnologie e Studio Radiazioni Extraterrestri, CNR, Bologna, Italy.
9 Astrophysikalisches Institut, Potsdam, Germany.
10 Astronomical Institute, CZ-251 65 Ondrejov, Czech Republic.
11 U. P. State Observatory, Manora Park, Naini Tal, 263 129 India.
12 Science Institute, University of Iceland, Reykjavik, Iceland.
13 Institut d'Astrophysique et de Géophysique de Liège, Université de Liège, 4000 Liege, Belgium.
14 Osservatorio Astronomico "V. Cerulli," Teramo, Italy.
15 Calar Alto Observatory, Almería, Spain.
16 Kitt Peak National Observatory, Tucson AZ, 85726, USA.
17 Astronomical Observatory, University of Bonn, Germany.
18 Radioastronomisches Institut, 53121 Bonn, Germany.
19 Max-Plank Institut für Astronomie, Heidelberg, Germany.
20 Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, and Beijing Astrophysics Center, Beijing 100871, China.
21 Nikolaev University Observatory, Nikolskaya, 24, 327030 Nikolaev, Ukraine.
22 Nikolaev Space Research Group, Nikolaev Astronomical Observatory, 327030 Nikolaev, Ukraine.
23 Space Research Organization Netherlands, Utrecht, The Netherlands.
24 Istituto di Astrofisica Spaziale, CNR, Frascati, Italy.
*   To whom correspondence should be addressed E-mail: ajct{at}laeff.esa.es


Read the Full Text





ADVERTISEMENT
Click Me!

ADVERTISEMENT
Click Me!

To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)