Comparing star formation on large scales in the c2d legacy clouds: Bolocam 1.1 mm dust continuum surveys of Serpens, Perseus, and Ophiuchus

@inproceedings{Enoch2007ComparingSF,
  title={Comparing star formation on large scales in the c2d legacy clouds: Bolocam 1.1 mm dust continuum surveys of Serpens, Perseus, and Ophiuchus},
  author={Melissa L. Enoch and Jason S. Glenn and Neal J. Evans and Anneila I. Sargent and Kaisa Elizabeth Young and T. L. Huard Caltech and Univ. of Colorado and Boulder and Univ. of Texas and Austin and Nicholls State Univ. and Cfa},
  year={2007}
}
We have undertaken an unprecedentedly large 1.1 mm continuum survey of three nearby star-forming clouds using Bolocam at the Caltech Submillimeter Observatory. We mapped the largest areas in each cloud at millimeter or submillimeter wavelengths to date: 7.5 deg2 in Perseus (Enoch and coworkers), 10.8 deg^2 in Ophiuchus (Young and coworkers), and 1.5 deg2 in Serpens with a resolution of 31", detecting 122, 44, and 35 cores, respectively. Here we report on results of the Serpens survey and… CONTINUE READING

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