Change in the chemical composition of infalling gas forming a disk around a protostar-Reference-Cited by-同舟云学术

Change in the chemical composition of infalling gas forming a disk around a protostar

Published:2014-02-12 Issue:7490 Volume:507 Page:78-80
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Sakai Nami,Sakai Takeshi,Hirota Tomoya,Watanabe Yoshimasa,Ceccarelli Cecilia,Kahane Claudine,Bottinelli Sandrine,Caux Emmanuel,Demyk Karine,Vastel Charlotte,Coutens Audrey,Taquet Vianney,Ohashi Nagayoshi,Takakuwa Shigehisa,Yen Hsi-Wei,Aikawa Yuri,Yamamoto Satoshi

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature13000.pdf

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3. Ohashi, N., Hayashi, M., Ho, P. T. P. & Momose, M. Interferometric imaging of IRAS04368+2557 in the L1527 molecular cloud core: a dynamically infalling envelope with rotation. Astrophys. J. 475, 211–223 (1997)

4. Shirley, Y. L., Evans, N. J., II & Rawlings, J. M. C. Tracing the mass during low-mass star formation. III. Models of the submillimeter dust continuum emission from class 0 protostars. Astrophys. J. 575, 337–353 (2002)

5. Yen, H.-W., Takakuwa, S., Ohashi, N. & Ho, P. T. P. Unveiling the evolutionary sequence from infalling envelopes to Keplerian disks around low-mass protostars. Astrophys. J. 772, 22 (2013)

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