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Global star formation in the L1630 molecular cloudThis paper presents the preliminary results of a study of star formation in the L1630 molecular cloud. An unbiased well sampled systematic CS (2 to 1) survey for density condensations and a 2.2-micron survey for embedded infrared sources in L1630 have been completed. These surveys have provided a complete census of the dense cores and young stellar objects within this molecular cloud. As a result, four embedded stellar clusters have been identified in this cloud. These clusters are located near the most massive CS cores implying that the most active sites of star formation are located within the most massive dense cores.
Document ID
19910068592
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lada, Elizabeth A.
(Texas, University Austin, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Astrophysics
Meeting Information
Meeting: Physical Processes in Fragmentation and Star Formation
Location: Rome
Country: Italy
Start Date: June 5, 1989
End Date: June 11, 1989
Sponsors: Universita di Roma I, Osservatorio Astrofisico di Arcetri, Osservatorio Astronomico di Roma, CNR
Accession Number
91A53215
Funding Number(s)
CONTRACT_GRANT: NGT-50320
Distribution Limits
Public
Copyright
Other

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