Hostname: page-component-cd9895bd7-lnqnp Total loading time: 0 Render date: 2024-12-25T15:41:34.655Z Has data issue: false hasContentIssue false
  • English
  • Français

YSOs in Taurus-Auriga-Perseus and Orion

Published online by Cambridge University Press:  21 March 2013

Sarolta Zahorecz ,
L. Viktor Tóth ,
Gábor Marton ,
Toshikazu Onishi ,
Lajos G. Balázs ,
Orsolya Fehér ,
Akiko Kawamura ,
Yoshimi Kitamura ,
Mónika Lisztes  and
Atsushi Nishimura
...Show all authors
Sarolta Zahorecz
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
L. Viktor Tóth
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
Gábor Marton
Affiliation:
Konkoly Observatory of the Hungarian Ac. of Sci., PO Box 67, 1525 Budapest, Hungary
Toshikazu Onishi
Affiliation:
Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, Osaka 599-8531, Japan
Lajos G. Balázs
Affiliation:
Konkoly Observatory of the Hungarian Ac. of Sci., PO Box 67, 1525 Budapest, Hungary
Orsolya Fehér
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
Akiko Kawamura
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Yoshimi Kitamura
Affiliation:
JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, Japan
Mónika Lisztes
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
Atsushi Nishimura
Affiliation:
Department of Physical Science, Osaka Prefecture University, Gakuen 1-1, Sakai, Osaka 599-8531, Japan
László Pásztor
Affiliation:
Research Institute for Soil Science and Agricultural Chemistry of the Hungarian Academy of Sciences, GIS Lab, Budapest, Hungary
Sándor Pintér
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
István Rácz
Affiliation:
Loránd Eötvös University, Departement of Astronomy, Pázmány Péter sétány 1, 1117 Budapest, Hungary, email: [email protected]
Motohide Tamura
Affiliation:
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
Rogel M.D. Sese
Affiliation:
College of Arts and Sciences, UPLB College, Laguna 4031Philippines
Munetaka Ueno
Affiliation:
JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510, 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.

Physical parameters were derived for 100 young stellar objects in the TAPO region.

Keywords

stars: formation — stars: pre–main-sequence — infrared: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 64
Copyright
Copyright © International Astronomical Union 2013

References

Ishihara, D., Onaka, T., Kataza, H.et al. 2010, A&A, 514, 1Google Scholar
Fazio, G. G., Hora, J. L., Allen, L. E.et al. 2004, ApJS, 154, 10Google Scholar
Rieke, G. H., Young, E. T., Engelbracht, C. W.et al. 2004, ApJS, 154, 25CrossRefGoogle Scholar
Kawada, M., Baba, H., Barthel, P. D., Clements, D.et al. 2007, PASJ, 59, 389Google Scholar
Robitaille, T. P., Whitney, B. A., Indebetouw, R., & Wood, K. 2007, ApJS, 169, 328CrossRefGoogle Scholar
Skrutskie, M. F., Cutri, R. M., Stiening, R.et al. 2006, AJ, 131, 1163CrossRefGoogle Scholar
Yamamura, I.et al. 2010, AKARI/FIS Bright Source Catalogue Version 1.0 Release NoteGoogle Scholar
Werner, M. W., Roellig, T. L., Low, F. J.et al. 2004, ApJS, 154, 1CrossRefGoogle Scholar
Wright, E. L., Eisenhardt, P. R. M., Mainzer, A. K.et al. 2010, AJ, 140, 1868CrossRefGoogle Scholar