PoWR

Theoretical spectral energy distributions (SEDs) from expanding NLTE model atmospheres for hot stars.

Identifier
Source	https://dc.g-vo.org/rr/q/lp/custom/org.gavo.dc/gvo/data/PoWR/powr.ipap
Related Identifier	http://dc.zah.uni-heidelberg.de/gvo/data/PoWR/powr.ipap/info
Related Identifier	http://www.astro.physik.uni-potsdam.de/~PoWR
Metadata Access	http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://org.gavo.dc/gvo/data/PoWR/powr.ipap

Provenance
Creator	Wolf-Rainer Hamann
Publisher	The GAVO DC team
Publication Year	2013
OpenAccess	true
Contact	GAVO Data Center Team <gavo(at)ari.uni-heidelberg.de>

Representation
Resource Type	Dataset
Discipline	Astrophysics and Astronomy; Cosmology; Natural Sciences; Physics; Stellar Astronomy