Mass loss of M supergiants Virtual Observatory Resource

Authors

1. Josselin E.
2. Blommaert J.A.D.L.
3. Groenewegen M.A.T.
4. Omont A.
5. Li F.L.

Published by

CDS

Abstract

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. <GCPD/39> and <GCPD/09>, respectively.

Keywords

1. supergiant-stars
2. m-stars
3. stellar-mass-loss
4. radio-astronomy
5. infrared-photometry

Bibliographic source Bibcode

2000A&A...357..225J

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/357/225

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/357/225

Document Object Identifer DOI

doi:10.26093/cds/vizier.33570225

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/357/225
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/357/225
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/357/225

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).