Thermal Methanol from 33 Clouds at 48 GHz Virtual Observatory Resource

Authors

1. Slysh V.I.
2. Bachiller R.
3. Berulis I.I.
4. Valtts I.E.
5. Gomez-Gonzalez J.,Kalenskii S.V.

Published by

CDS

Abstract

A search for thermal emission in the 1_0_-0_0_A^+^ methanol line was made at a frequency of 48.4GHz toward many celestial molecular clouds. The line was found in 33 clouds, and the methanol abundance varied over a large interval from 10^-9^ to 10^-7^.

Keywords

1. interstellar-medium
2. astrophysical-masers
3. radio-astronomy

Bibliographic source Bibcode

1994AZh....71...37S

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/71/37

IVOA Identifier IVOID

ivo://CDS.VizieR/J/AZh/71/37

Access

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http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/71/37
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/71/37
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/71/37

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Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

IVOA Cone Search SCS

For use with a cone search client (e.g., TOPCAT).
http://vizier.cds.unistra.fr/viz-bin/conesearch/J/AZh/71/37/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/AZh/71/37/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/71/37/table1?