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Interstellar hydroxyl near Sagittarius B2

Journal Article · · Sov. Astron. Lett. (Engl. Transl.); (United States)
OSTI ID:5867673
The 1665-, 1667-MHz OH absorption lines near the radio source Sgr B2 have been observed with the RATAN-600 radio telescope at 2'.2 x 47' x 5.4 km/sec resolution. Physical parameters are determined for the five OH clouds observed in this direction at positive radial velocities. Evidently only one of these clouds can have any connection with the Sgr B2 source; it is located at the edge of the gas envelope surrounding that source.
Research Organization:
Special Astrophysical Observatory, USSR Academy of Sciences, Nizhnii Arkhyz
OSTI ID:
5867673
Journal Information:
Sov. Astron. Lett. (Engl. Transl.); (United States), Journal Name: Sov. Astron. Lett. (Engl. Transl.); (United States) Vol. 7:3; ISSN SALED
Country of Publication:
United States
Language:
English

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