X-ray emission of T Tau stars in Lupus 3

DOI

I present analysis results of an XMM-Newton observation of the Lupus 3 region that contains a high proportion of young low mass T Tauri stars in the Lupus star-forming complex. The detection of X-ray sources in 0.5 to 4.5-keV images of the Lupus 3 core was performed using the standard source detection method of the XMM-Newton Science Analysis Software. One hundred and two candidate X-ray sources were detected in the 30-arcmin diameter field-of-view of the EPIC cameras, of which 25 have visible or near-IR counterparts that are known as pre-main sequence stars.

Cone search capability for table J/A+A/454/595/table6 (X-ray sources in the core of the Lupus 3 region)

Identifier
DOI http://doi.org/10.26093/cds/vizier.34540595
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/454/595
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/454/595
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/454/595
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/454/595
Provenance
Creator Gondoin P.
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