The Extinction Law in High-Redshift Galaxies

Muñoz, J. A.; Falco, E. E.; Kochanek, C. S.; McLeod, B. A.; Mediavilla, E.
Referencia bibliográfica

The Astrophysical Journal, Volume 605, Issue 2, pp. 614-619.

Fecha de publicación:
4
2004
Número de autores
5
Número de autores del IAC
1
Número de citas
45
Número de citas referidas
41
Descripción
We estimate the dust extinction laws in two intermediate-redshift galaxies. The dust in the lens galaxy of LBQS 1009-0252, which has an estimated lens redshift of zl~=0.88, appears to be similar to that of the SMC, with no significant feature at 2175 Å. Only if the lens galaxy is at a redshift of zl~=0.3, which is completely inconsistent with the galaxy colors, luminosity, and location on the fundamental plane, can the data be fitted with a normal Galactic extinction curve. The dust in the zl=0.68 lens galaxy for B028+357, whose reddened image lies behind a molecular cloud, requires a very flat ultraviolet extinction curve with (formally) RV=12+/-2. Both lens systems seem to have unusual extinction curves by Galactic standards. Based on observations made with the NASA/ESA Hubble Space Telescope. The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS5-26555.