GM 2-4 H_2_ emission-line objects Virtual Observatory Resource

Authors

1. Khanzadyan T.
2. Movsessian T.A.
3. Davis C.J.
4. Magakian T.Yu.
5. Gredel R.,Nikogossian E.H.

Published by

CDS

Abstract

We present a multi-wavelength study of the region towards the GM 2-4 nebula and the nearby source IRAS 05373+2340. Our near-infrared H_2_ 1-0 S(1) line observations reveal various shock-excited features which are part of several bipolar outflows. We identify candidates for the driving sources of the outflows from a comparison of the multi-waveband archival data sets and spectral energy distribution (SED) modelling. The SED spectral slope ({alpha}^IRAC^) for all the protostars in the field was then compared with the visual extinction map. This comparison suggests that star formation progresses from north-east to south-west across this region.

Keywords

1. molecular-clouds
2. infrared-sources

Bibliographic source Bibcode

2011MNRAS.418.1994K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/418/1994

IVOA Identifier IVOID

ivo://CDS.VizieR/J/MNRAS/418/1994

Document Object Identifer DOI

doi:10.26093/cds/vizier.74181994

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/418/1994
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/418/1994
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/418/1994

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
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).
https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/418/1994/table1?
https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/418/1994/table1?
http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/418/1994/table1?