Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244..102c&link_type=abstract
Astrophysical Journal, Part 1, vol. 244, Feb. 15, 1981, p. 102-114. Research supported by the Consejo Nacional de Ciencia y Tec
Astronomy and Astrophysics
Astrophysics
152
Carbon Monoxide, Herbig-Haro Objects, Interstellar Gas, Molecular Clouds, Nebulae, Variable Stars, Astronomical Maps, Emission Spectra, Magnetohydrodynamic Flow, Stellar Winds
Scientific paper
R Mon is described as a peculiar star located at the apex of the (apparent) cometary nebula NGC 2261. Carbon monoxide observations of this region show an elongated molecular cloud with R Mon at the center. The suggestion is made that the cloud is disk shaped and that the stellar wind of R Mon has created a bipolar cavity in it. The results show that a recently formed, wind-producing star located in a disklike molecular environment (interstellar disk) will have its wind channeled in two opposite directions along the poles of the disk.
Barral J. F.
Cantó Jorge
Carral Patricia
Rodriguez Luis F.
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