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Table · dataset · 2000

Mass loss of M supergiants

Listed in IVOA Registry (Virtual Observatory)

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.

Description

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.

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Where it is published

Documentation and papers

Catalogue records · 2

Topics

Stated by source
Infrared · Radio
Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/357/22512 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:infraredsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0