Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-14T23:13:34.430Z Has data issue: false hasContentIssue false
  • English
  • Français

Line surveys of irradiated protostars: Photo-destruction and evaporation

Published online by Cambridge University Press:  18 July 2017

Johan E. Lindberg ,
Steven B. Charnley ,
Jes K. Jørgensen ,
Yoshimasa Watanabe ,
Suzanne E. Bisschop ,
Nami Sakai  and
Satoshi Yamamoto
Johan E. Lindberg
Affiliation:
NASA Goddard Space Flight Center, Astrochemistry Laboratory, Mail Code 691, 8800 Greenbelt Road, Greenbelt, MD 20771, USA email: [email protected]
Steven B. Charnley
Affiliation:
NASA Goddard Space Flight Center, Astrochemistry Laboratory, Mail Code 691, 8800 Greenbelt Road, Greenbelt, MD 20771, USA email: [email protected]
Jes K. Jørgensen
Affiliation:
Centre for Star and Planet Formation, Niels Bohr Institute and Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, DK-1350 Copenhagen K, Denmark
Yoshimasa Watanabe
Affiliation:
Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
Suzanne E. Bisschop
Affiliation:
Centre for Star and Planet Formation, Niels Bohr Institute and Natural History Museum of Denmark, University of Copenhagen, Øster Voldgade 5-7, DK-1350 Copenhagen K, Denmark
Nami Sakai
Affiliation:
Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198, Japan
Satoshi Yamamoto
Affiliation:
Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo, 113-0033, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Submillimetre observations of the externally irradiated protostar R CrA IRS7B show that this source has dramatically different chemical abundances in comparison with otherwise similar embedded protostars not subject to external irradiation.

Keywords

stars: formationISM: moleculesISM: abundancesastrochemistry
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E25
Copyright
Copyright © International Astronomical Union 2017 

References

Cazaux, S., Tielens, A. G. G. M., Ceccarelli, C., et al. 2003, ApJ Lett., 593, L51 CrossRefGoogle Scholar
Lindberg, J. E. & Jørgensen, J. K., 2012, A&A., 548, A24 Google Scholar
Lindberg, J. E., Jørgensen, J. K., Green, J. D., et al. 2014, A&A., 565, A29 Google Scholar
Lindberg, J. E., Jørgensen, J. K., Watanabe, Y., et al. 2015, A&A., in press (arXiv:1509.02514)Google Scholar
Sakai, N. & Yamamoto, S., 2013, Chemical Reviews, 113, 8981 Google Scholar