21-cm observations of the CEP IV star-formation region

Details 21-cm observations of the CEP IV star-formation region 21-cm observations of the CEP IV star-formation region

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85.1631g&link_type=abstract

Astronomical Journal, vol. 85, Dec. 1980, p. 1631-1637. Research supported by the University of Nevada.

Astronomy and Astrophysics

Astronomy

5

Hydrogen Clouds, Interstellar Gas, Radio Astronomy, Star Formation, Autocorrelation, Nebulae, Radio Sources (Astronomy), Stellar Motions, Supernovae, T Tauri Stars

Scientific paper

The Cep IV star-formation region has been mapped at 21 cm. The resulting
H I distribution indicates that the available gas forms a broken ring
coincident with the optical nebulosity. Comparison of this feature with
other kinematic data for both stars and gas suggests that sequential
star formation is an ongoing process in this region.

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