MIPS 24um nebulae (Gvaramadze+, 2010)

Details MIPS 24um nebulae (Gvaramadze+, 2010) MIPS 24um nebulae (Gvaramadze+, 2010)

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74051047g&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/405/1047. Originally published in: 2010MNRAS.405.1047G

Computer Science

Nebulae, Millimetric/Submm Sources, Photometry: Infrared

Scientific paper

Massive evolved stars lose a large fraction of their mass via copious stellar wind or instant outbursts. During certain evolutionary phases, they can be identified by the presence of their circumstellar nebulae. In this paper, we present the results of a search for compact nebulae (reminiscent of circumstellar nebulae around evolved massive stars) using archival 24um data obtained with the Multiband Imaging Photometer for Spitzer. We have discovered 115 nebulae, most of which bear a striking resemblance to the circumstellar nebulae associated with luminous blue variables (LBVs) and late WN-type (WNL) Wolf-Rayet (WR) stars in the Milky Way and the Large Magellanic Cloud (LMC).
(1 data file).

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