Published in

American Astronomical Society, Astrophysical Journal Supplement, 2(173), p. 377-391, 2007

DOI: 10.1086/522932

Links

Tools

Export citation

Search in Google Scholar

Ultraviolet, Optical, and Infrared Constraints on Models of Stellar Populations and Dust Attenuation

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Green circle
Published version: archiving allowed
Data provided by SHERPA/RoMEO
Beta version