Molecular clouds in Cepheus and Cassiopeia (Yonekura+ 1997)

Details Molecular clouds in Cepheus and Cassiopeia (Yonekura+ 1997) Molecular clouds in Cepheus and Cassiopeia (Yonekura+ 1997)

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ycat..21100021y&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/110/21. Originally published in: 1997ApJS..110...21Y

Astronomy and Astrophysics

Astronomy

Co, Interstellar Medium

Scientific paper

A large-scale ^13CO(J=1-0) survey for nearby molecular clouds was performed toward the Cepheus and Cassiopeia regions (100°=1.8K.km/s=3σ) is detected at 1015 positions. On the basis of the 13CO data, 188 distinct 13CO clouds are identified whose total mass is 1.0x105M&sun;. Physical properties of the 13CO clouds such as molecular column densities, sizes, and masses are derived for each cloud. Astronomical objects associated with the 13CO clouds were searched for in the literature: 10 H II regions, eight reflection nebulae, 23 T Tauri type stars, 28 molecular outflows, and 125 IRAS point sources selected as candidates for protostars are likely to be associated with the 13CO clouds. (3 data files).

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