A Case Study of Low-Mass Star Formation

This article synthesizes observational data from an extensive program aimed toward a comprehensive understanding of star formation in a low-mass star-forming molecular cloud. New observations and published data spanning from the centimeter wave band to the near infrared reveal the high and low densi...

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Veröffentlicht in:	arXiv.org 2007-06
Hauptverfasser:	Swift, J, Welch, Wm J
Format:	Artikel
Sprache:	eng
Schlagworte:	Centimeter waves Low mass stars Molecular clouds Molecular gases Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Pre-main sequence stars Star & galaxy formation Star formation
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Beschreibung
Zusammenfassung:	This article synthesizes observational data from an extensive program aimed toward a comprehensive understanding of star formation in a low-mass star-forming molecular cloud. New observations and published data spanning from the centimeter wave band to the near infrared reveal the high and low density molecular gas, dust, and pre-main sequence stars in L1551.
ISSN:	2331-8422
DOI:	10.48550/arxiv.0706.2206