Star formation in Lynds 1641
We conducted an extensive multi-wavelength study of the nearest giant molecular cloud, L1641, with the goal of characterizing its stellar populations. At a distance of approximately 500 pc, L1641 provides an excellent opportunity for studying star formation over the entire range of stellar masses, a...
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Language: | ENG |
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ScholarWorks@UMass Amherst
1996
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Online Access: | https://scholarworks.umass.edu/dissertations/AAI9619366 |