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Post Info TOPIC: Lynds 988e


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Posts: 131433
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RE: Lynds 988e
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Title: Spitzer, Near-Infrared, and Submillimeter Imaging of the Relatively Sparse Young Cluster, Lynds 988e
Authors: Thomas S. Allen, Judith L. Pipher, Robert A. Gutermuth, S. Thomas Megeath, Joseph D. Adams, Terry L. Herter, Jonathan P. Williams, Jennifer A. Goetz-Bixby, Lori E. Allen, Philip C. Myers
(Version v2)

We present {\it Spitzer} images of the relatively sparse, low luminosity young cluster L988e, as well as complementary near-infrared (NIR) and submillimeter images of the region. The cluster is asymmetric, with the western region of the cluster embedded within the molecular cloud, and the slightly less dense eastern region to the east of, and on the edge of, the molecular cloud. With these data, as well as with extant H\alpha data of stars primarily found in the eastern region of the cluster, and a molecular ^{13}CO gas emission map of the entire region, we investigate the distribution of forming young stars with respect to the cloud material, concentrating particularly on the differences and similarities between the exposed and embedded regions of the cluster. We also compare star formation in this region to that in denser, more luminous and more massive clusters already investigated in our comprehensive multi-wavelength study of young clusters within 1 kpc of the Sun.

Read more (410kb, PDF)

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L

Posts: 131433
Date:
Permalink  
 

Title: Spitzer, Near-Infrared, and Submillimeter Imaging of the Relatively Sparse Young Cluster, Lynds 988e
Authors: Thomas S. Allen, Judith L. Pipher, Robert A. Gutermuth, S. Thomas Megeath, Joseph D. Adams, Terry L. Herter, Jonathan P. Williams, Jennifer A. Goetz-Bixby, Lori E. Allen, Philip C. Myers

We present {\it Spitzer} images of the relatively sparse, low luminosity young cluster L988e, as well as complementary near-infrared (NIR) and submillimeter images of the region. The cluster is asymmetric, with the western region of the cluster embedded within the molecular cloud, and the slightly less dense eastern region to the east of, and on the edge of, the molecular cloud. With these data, as well as with extant H\alpha data of stars primarily found in the eastern region of the cluster, and a molecular ^{13}CO gas emission map of the entire region, we investigate the distribution of forming young stars with respect to the cloud material, concentrating particularly on the differences and similarities between the exposed and embedded regions of the cluster. We also compare star formation in this region to that in denser, more luminous and more massive clusters already investigated in our comprehensive multi-wavelength study of young clusters within 1 kpc of the Sun.

Read ore  (410kb, PDF)

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