Optical Observations of Afterglows

dc.creatorPian, Elena
dc.date2001-10-02
dc.date2002-07-28
dc.date.accessioned2026-07-07T02:00:31Z
dc.date.available2026-07-07T02:00:31Z
dc.descriptionOptical, infrared and ultraviolet observations of GRB fields have allowed detection of counterparts and host galaxies of the high energy transients, thus crucially contributing to our present knowledge of the GRB phenomenon. Measurements of afterglow variable emission, polarized light, redshifted absorption and emission line spectra, as well as host galaxies brightnesses and colors have clarified many fundamental issues related to the radiation mechanisms and environments of GRBs, setting the background towards disclosing the nature of their progenitors.
dc.description22 pages, Latex, 6 PostScript figures, Chapter for the book "Supernovae and Gamma-Ray Bursters", edited by K. W. Weiler, Lecture Notes in Physics, Springer-Verlag Press (2001) (text and Table 1 updated with respect to formerly submitted version)
dc.identifierhttps://arxiv.org/abs/astro-ph/0110051
dc.identifierhttp://arxiv.org/abs/astro-ph/0110051
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3447
dc.subjectAstrophysics
dc.titleOptical Observations of Afterglows
dc.typetext

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