Star Formation in the Gulf of Mexico
arXiv:1101.4670 · doi:10.1051/0004-6361/200912671
Abstract
We present an optical/infrared study of the dense molecular cloud, L935, dubbed "The Gulf of Mexico", which separates the North America and the Pelican nebulae, and we demonstrate that this area is a very active star forming region. A wide-field imaging study with interference filters has revealed 35 new Herbig-Haro objects in the Gulf of Mexico. A grism survey has identified 41 Halpha emission-line stars, 30 of them new. A small cluster of partly embedded pre-main sequence stars is located around the known LkHalpha 185-189 group of stars, which includes the recently erupting FUor HBC 722.
Submitted to A&A, 14 pages, 18 figures
References in corpus (1)
Cited by in corpus (15)
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- The Villafranca catalog of Galactic OB groups: I. Systems with O2-O3.5 stars
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- A ZTF Look at Optical Variability of Young Stellar Objects in the North America and Pelican Nebulae Complex
- Outflows, Dusty Cores, and a Burst of Star Formation in the North America and Pelican Nebulae
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- Long-term BVRI photometric light curves of 15 PMS stars in the IC 5070 star-forming region
- LAMOST MRS-N Observations of the W80 Region