The structure of interstellar hydroxyl masers - VLBI synthesis observations of W3/OH/

Details The structure of interstellar hydroxyl masers - VLBI synthesis observations of W3/OH/ The structure of interstellar hydroxyl masers - VLBI synthesis observations of W3/OH/

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...239...89r&link_type=abstract

Astrophysical Journal, Part 1, vol. 239, July 1, 1980, p. 89-99, 101-103, 105-111.

Astronomy and Astrophysics

Astrophysics

204

Hydrogen Clouds, Hydroxyl Emission, Interstellar Masers, Very Long Base Interferometry, Astronomical Catalogs, Astronomical Photography, Line Spectra, Nebulae, Protostars, Zeeman Effect

Scientific paper

The results of an extensive investigation of the 1665 MHz OH emission from W3(OH) are discussed. Interstellar OH masers are probably found in sources which span a range of evolutionary states. Synthesis maps of W75(N), for example, indicate that the OH emission comes from a region with dynamical properties more complex than found in W3(OH) (Haschick et al., 1980).

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