Mass loss of M supergiants (Josselin+, 2000)

Details Mass loss of M supergiants (Josselin+, 2000) Mass loss of M supergiants (Josselin+, 2000)

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..33570225j&link_type=abstract

VizieR On-line Data Catalog: J/A+A/357/225. Originally published in: 2000A&A...357..225J

Physics

Stars: Supergiant, Stars: M-Type, Mass Loss, Radio Lines, Photometry: Infrared

Scientific paper

The following tables present near-infrared photometry and millimeter observations of a sample of optical M supergiants, together with estimations of their luminosity and dust mass-loss rate. Near-infrared observations were done in February 1995 with the ESO T2.2m-IRAC1 and T3.6m-TIMMI instruments, millimeter observations were made in December 1994 with the IRAM-30m-telescope and in February 1995 with the SEST. For a description of the (N1-N3) and (JHKL) photometric system, see e.g. and , respectively. (3 data files).

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