Young (proto)stellar population in L1630 (Mookerjea+ 2009)

Physics

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H Ii Regions, Ysos, Photometry: Infrared

Scientific paper

The observations of NGC 2023 MM 1/MM 2 were made on Dec. 13, 1999 and April 13, 2000 using one frequency setting in the C-array configuration of the Berkeley-Illinois-Maryland Association (BIMA) interferometric array.
We obtained several large scan maps (8'x8') of the NGC 2023 region with the Submillimeter Common User Bolometer Array (SCUBA) on JCMT during SCUBA commissioning time on four nights in December, 1997.
(3 data files).

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