Orion Nebula Cluster proplyd candidates (Kastner+, 2005)

Details Orion Nebula Cluster proplyd candidates (Kastner+, 2005) Orion Nebula Cluster proplyd candidates (Kastner+, 2005)

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..21600511k&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/160/511. Originally published in: 2005ApJS..160..511K

Computer Science

1

Clusters: Open, Interstellar Medium, Stars: Pre-Main Sequence, X-Ray Sources

Scientific paper

We investigate the X-ray and near-infrared emission properties of a sample of pre-main-sequence (PMS) stellar systems in the Orion Nebula Cluster (ONC) that display evidence for circumstellar disks ("proplyds") and optical jets in Hubble Space Telescope (HST) imaging. Our study uses X-ray data acquired during Chandra Orion Ultradeep Program (COUP) observations, as well as complementary optical and near-infrared data recently acquired with HST and the Very Large Telescope (VLT), respectively.
(3 data files).

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