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- W1966856727 abstract "Abstract Eleven low-mass cores are found in the Orion Molecular Cloud 2 from VLA observations of the line emission of NH3 (1,1). They are perhaps clumps prior to gravitatonal collapse with average radius of 0.03 pc and mass of 3.5 M⊙, distributed along the central axes of filaments in the NS direction. We find a velocity gradient of ∼ 5 km s−1 pc−1 in the declination direction within a 3′ region. Based on our NH3(1,1) observations and compared with dust continuum emission at millimilion wavelength as well as in the infrared, we suggest that most of these dense cores are probably protosteller condensations, not yet containing stellar cores, but are self-gravitating systems in thermodynamical equilibrium." @default.
- W1966856727 created "2016-06-24" @default.
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- W1966856727 date "1995-10-01" @default.
- W1966856727 modified "2023-09-24" @default.
- W1966856727 title "Physical and dynamical properties of a low-mass star-forming region" @default.
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- W1966856727 doi "https://doi.org/10.1016/0275-1062(95)00062-w" @default.
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