http://www.cnr.it/ontology/cnr/individuo/prodotto/ID5701
The blue host galaxy of the red GRB 000418 (Articolo in rivista)
- Type
- Label
- The blue host galaxy of the red GRB 000418 (Articolo in rivista) (literal)
- Anno
- 2003-01-01T00:00:00+01:00 (literal)
- Alternative label
Gorosabel J., Klose S., Christensen L., Fynbo J.P.U., Hjorth J., Greiner J., Tanvir N., Jensen B.L., Pedersen H., Holland S.T., Lund N., Jaunsen A.O., Castro Ceron J.M., Castro-Tirado A.J., Fruchter A., Pian E., Vreeswijk P.M., Burud I., et al (2003)
The blue host galaxy of the red GRB 000418
(literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- Gorosabel J., Klose S., Christensen L., Fynbo J.P.U., Hjorth J., Greiner J., Tanvir N., Jensen B.L., Pedersen H., Holland S.T., Lund N., Jaunsen A.O., Castro Ceron J.M., Castro-Tirado A.J., Fruchter A., Pian E., Vreeswijk P.M., Burud I., et al (literal)
- Pagina inizio
- Pagina fine
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
- Note
- ISI Web of Science (WOS) (literal)
- Titolo
- The blue host galaxy of the red GRB 000418 (literal)
- Abstract
- We report on multi-band (UBVRIZJ_{s}K_{s})
observations of the host galaxy
of the April 18, 2000 gamma-ray burst. The
Spectral Energy Distribution
(SED) is analysed by fitting empirical and
synthetic spectral templates.
We find that: (i) the best SED fit is
obtained with a starburst template,
(ii) the photometric redshift is consistent
with the spectroscopic
redshift, (iii) the colours of the host are
inconsistent with an old
stellar population, and (iv) the global
extinction is constrained to be in
the range A_{V}=0.12-0.61 mag. The derived
global extinction agrees with
the one reported for the afterglow (A_{V} =
0.4-0.9 mag), suggesting a
homogeneous distribution of the
interstellar medium (ISM) in the host
galaxy. These findings are supplemented by
morphological information from
Hubble Space Telescope (HST) imaging: the
surface brightness profile is
smooth, symmetric and compact with no
underlying structures (like dust
lanes, spiral arms or disks). A natural
scenario which accounts of all the
above results is a nuclear starburst that
harbours a young population of
stars from which the GRB originated. (literal)
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