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Density structure of dense cores in the Cepheus molecular cloud

Published online by Cambridge University Press:  03 August 2017

K. Sunada ,
T. Hasegawa ,
M. Hayashi ,
Y. Fukui  and
K. Sugitani
K. Sunada
Affiliation:
Department of Astronomy, University of Tokyo
T. Hasegawa
Affiliation:
Institute of Astronomy, University of Tokyo
M. Hayashi
Affiliation:
Department of Astronomy, University of Tokyo
Y. Fukui
Affiliation:
Department of Astrophysics, Nagoya University
K. Sugitani
Affiliation:
College of General Education, Nagoya City University

Extract

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We mapped 5 dense cores in the Cepheus molecular cloud in the optically thin C18O (J = 1 — 0) line using the 45-m telescope at Nobeyama and derived density profiles around those cores assuming spherical symmetry. Cloud cores are selected from the 13CO (J = 1 — 0) map obtained through the unbiased survey program with the 4-m telescope at Nagoya university.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 500 - 501
Copyright
Copyright © Kluwer 1991