Chandra obs. of Serpens star-forming region

DOI

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.

Cone search capability for table J/A+A/463/275/table5 (X-ray sources detected with PWDETECT in the Chandra observation of the Serpens star forming region.)

Cone search capability for table J/A+A/463/275/table6 (The cross-identification of the sources below was obtained from the Simbad database, with a search radius of 5 arcsec.)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34630275
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/463/275
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/463/275
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/463/275
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/463/275
Provenance
Creator Giardino G.; Favata F.; Micela G.; Sciortino S.; Winston E.
Publisher CDS
Publication Year 2007
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Cosmology; Interstellar medium; Natural Sciences; Physics; Stellar Astronomy