Kutner et al. 1976
Kutner, M.L., N.J. Evans, II, and K.D. Tucker, 1976: A dense molecular cloud in the OMC-1/OMC-2 region. Astrophys. J., 209, 452-457, doi:10.1086/154739.
H2CO emission at 2 mm is seen over a region 30' in extent which includes OMC-1 and OMC-2. The mass of this cloud, estimated from H2CO and CO observations, is ~ 7×103 M☉. The velocity pattern is one of rotation, with evidence for fragmentation into two or three distinct condensations. A sharp boundary to the molecular cloud is observed at the edge of the H II region in NGC 1977. It appears likely that NGC 1977 is a condensation at the northern end of the cloud, complementary to the Orion Nebula at the southern end.
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Kutner, M.L., Evans, N.J., II, and Tucker, K.D.: A dense molecular cloud in the OMC-1/OMC-2 region, Astrophys. J., 209, 452-457, doi:10.1086/154739, 1976.
Kutner, M.L., N.J. Evans, II, and K.D. Tucker (1976), A dense molecular cloud in the OMC-1/OMC-2 region, Astrophys. J., 209, 452-457, doi:10.1086/154739.
Kutner, M.L., N.J. Evans, II, and K.D. Tucker, 1976: A dense molecular cloud in the OMC-1/OMC-2 region. Astrophys. J., 209, 452-457, doi:10.1086/154739.
Kutner, M.L., Evans, N.J., II, & Tucker, K.D. 1976, Astrophys. J., 209, 452, doi:10.1086/154739.
Kutner ML, Evans NJ II, Tucker KD. A dense molecular cloud in the OMC-1/OMC-2 region, Astrophys J 1976;209:452-457. doi:10.1086/154739.
M.L. Kutner, N.J. Evans, II, K.D. Tucker, Astrophys. J. 209, 452-457, doi:10.1086/154739 (1976).