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Resource Record Summary

Catalog Service:
NGC 7129 pre-main sequence stars

Short name: J/A+A/507/227
IVOA Identifier: ivo://CDS.VizieR/J/A+A/507/227
DOI (Digital Object Identifier): 10.26093/cds/vizier.35070227
Publisher: CDS[+][Pub. ID]
More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/507/227
VO Compliance: Level 2: This is a VO-compliant resource.
Status: active
Registered: 2010 Oct 11 07:51:21Z
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Description


The reflection nebula NGC 7129 has long been known to be a site of recent star formation as shown, e.g., by the presence of deeply embedded protostars and HH objects. However, studies of the stellar population produced in the star formation process have remained rudimentary. A major step forward has been made with recent Spitzer imaging of the region. This study represents the next step towards a systematic assessment of the pre-main sequence population in NGC 7129. Completeness of the pre-main sequence sample is necessary for studying key features that allow the star-forming process to be understood, such as disk evolution, dynamical evolution, and mass function. At a presumed age of ~3Myr, NGC 7129 is in the critical range where disks around young stars disappear.

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under Cooperative Agreement AST0122449 with the Johns Hopkins University
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