Membership of the Orion Nebula population from the Chandra Orion Ultradeep Project

Konstantin V. Getman, Eric Feigelson, Nicolas Grosso, Mark J. Mccaughrean, Giusi Micela, Patrick Sean Broos, Gordon Garmire, Leisa K. Townsley

Research output: Contribution to journalArticle

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Abstract

The Chandra Orion Ultradeep project (COUP) observation described in a companion paper by Getman et al. provides an exceptionally deep X-ray survey of the Orion Nebula Cluster and associated embedded young stellar objects. Membership of the region is important for studies of the stellar IMF, cluster dynamics, and star formation. The COUP study detected 1616 X-ray sources. In this study we confirm cloud membership for 1315 stars, identify 16 probable foreground field stars having optical counterparts with discrepant proper motions, and classify the remaining 285 X-ray sources, of which 51 are lightly and 234 heavily obscured. The 51 lightly obscured sources without known counterparts fall into three groups: (i) 16 are likely new members of the Orion Nebula Cluster; (ii) 2 with unusually soft and nonflaring X-ray emission appear to be associated with nebular shocks, and may be new examples of X-rays produced at the bow shocks of Herbig-Haro outflows; (iii) the remaining 33 are very weak uncertain sources, possibly spurious. Out of 234 heavily absorbed sources without optical or near-infrared counterparts 75 COUP sources are likely new embedded cloud members (with membership for 42 confirmed by powerful X-ray flares), and the remaining 159 are likely extragalactic active galactic nuclei seen through the molecular cloud, as argued by a careful simulation of the extragalactic background population. Finally, a few new binary companions to Orion stars may have been found, but most cases of proximate COUP sources can be attributed to chance super-positions in this crowded field.

Original languageEnglish (US)
Pages (from-to)353-378
Number of pages26
JournalAstrophysical Journal, Supplement Series
Volume160
Issue number2
DOIs
StatePublished - Oct 1 2005

Fingerprint

Orion nebula
x rays
shock
stars
IMF
star distribution
proper motion
bows
project
molecular clouds
near infrared
active galactic nuclei
outflow
flares
star formation
simulation

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

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abstract = "The Chandra Orion Ultradeep project (COUP) observation described in a companion paper by Getman et al. provides an exceptionally deep X-ray survey of the Orion Nebula Cluster and associated embedded young stellar objects. Membership of the region is important for studies of the stellar IMF, cluster dynamics, and star formation. The COUP study detected 1616 X-ray sources. In this study we confirm cloud membership for 1315 stars, identify 16 probable foreground field stars having optical counterparts with discrepant proper motions, and classify the remaining 285 X-ray sources, of which 51 are lightly and 234 heavily obscured. The 51 lightly obscured sources without known counterparts fall into three groups: (i) 16 are likely new members of the Orion Nebula Cluster; (ii) 2 with unusually soft and nonflaring X-ray emission appear to be associated with nebular shocks, and may be new examples of X-rays produced at the bow shocks of Herbig-Haro outflows; (iii) the remaining 33 are very weak uncertain sources, possibly spurious. Out of 234 heavily absorbed sources without optical or near-infrared counterparts 75 COUP sources are likely new embedded cloud members (with membership for 42 confirmed by powerful X-ray flares), and the remaining 159 are likely extragalactic active galactic nuclei seen through the molecular cloud, as argued by a careful simulation of the extragalactic background population. Finally, a few new binary companions to Orion stars may have been found, but most cases of proximate COUP sources can be attributed to chance super-positions in this crowded field.",
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Membership of the Orion Nebula population from the Chandra Orion Ultradeep Project. / Getman, Konstantin V.; Feigelson, Eric; Grosso, Nicolas; Mccaughrean, Mark J.; Micela, Giusi; Broos, Patrick Sean; Garmire, Gordon; Townsley, Leisa K.

In: Astrophysical Journal, Supplement Series, Vol. 160, No. 2, 01.10.2005, p. 353-378.

Research output: Contribution to journalArticle

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