YSOs in DROXO (Deep rho Oph XMM obs.) Virtual Observatory Resource

Authors

1. Pillitteri I.
2. Sciortino S.
3. Flaccomio E.
4. Stelzer B.
5. Micela G.,Damiani F.
6. Testi L.
7. Montmerle T.
8. Grosso N.
9. Favata F.
10. Giardino G.

Published by

CDS

Abstract

X-rays from very young stars are powerful probes to investigate the mechanisms at work in the very first stages of the star formation and the origin of X-ray emission in very young stars. We present results from a 500ks long observation of the rho Ophiuchi cloud with a XMM-Newton large program named DROXO, aiming at studying the X-ray emission of deeply embedded young stellar objects (YSOs).

Keywords

1. x-ray-sources
2. young-stellar-objects
3. infrared-photometry

Bibliographic source Bibcode

2010A&A...519A..34P

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https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/519/A34

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/519/A34

Document Object Identifer DOI

doi:10.26093/cds/vizier.35190034

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