Chandra obs. of Serpens star-forming region Virtual Observatory Resource

Authors

1. Giardino G.
2. Favata F.
3. Micela G.
4. Sciortino S.
5. Winston E.

Published by

CDS

Abstract

To study the properties of X-ray emission from young stellar objects (YSOs) through their evolution from Class I to Class III and determine whether Class 0 protostars emit X-rays. A deep Chandra X-ray observation of the Serpens star-forming region was obtained. The Serpens Cloud Core is ideally suited for this type of investigation, being populated by a dense and extremely young cluster whose members are found in all evolutionary stages, including six well-studied Class 0 sources.

Keywords

1. stellar-associations
2. young-stellar-objects
3. pre-main-sequence-stars
4. x-ray-sources

Bibliographic source Bibcode

2007A&A...463..275G

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/463/275

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/463/275

Document Object Identifer DOI

doi:10.26093/cds/vizier.34630275

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/463/275
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/463/275
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/463/275

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