Discovering Protostars and their Host Clusters via WISE
Daniel J. Majaess

TL;DR
This study uses WISE infrared data to identify and analyze large samples of protostars and their host clusters across the sky, enhancing understanding of star formation regions.
Contribution
It introduces a hybrid infrared selection scheme to detect over 10,000 candidate protostars and correlates a subset with known star-forming regions, expanding the catalog of YSOs.
Findings
Detected over 10,000 candidate YSOs with WISE data.
Correlated ~200 protostar clusters with existing star-forming region catalogs.
Forthcoming surveys will improve detection and characterization of YSOs.
Abstract
A hybrid JHKs-W1W2W3W4 high-spectral index (alpha) selection scheme was employed to identify (sub)clusters of class I/f candidate protostars (YSOs) in WISE observations (the Wide-Field Infrared Survey Explorer). n>10^4 candidate YSOs were detected owing to WISE's advantageous all-sky spatial coverage, and a subsample (n~200) of their heavily-obscured host (sub)clusters were correlated with the Avedisova (2002) and Dias et al. (2002) catalogs of star-forming regions. Forthcoming observations from the VVV/UKIDSS surveys shall facilitate the detection of additional protostars and bolster efforts to delineate the Galactic plane, since the campaigns aim to secure deep JHKs photometry for a pertinent fraction of the WISE targets lacking 2MASS detections, and to provide improved data for YSOs near the limits of the 2MASS survey.
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