Sequential star formation at the periphery of the H II regions Sh 217 and Sh 219-Reference-Cited by-同舟云学术

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Sequential star formation at the periphery of the H II regions Sh 217 and Sh 219

Published:2003-02-14 Issue:3 Volume:399 Page:1135-1145
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Deharveng L.,Zavagno A.,Salas L.,Porras A.,Caplan J.,Cruz-González I.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20021841/pdf

Reference70 articles.

1. Polycyclic aromatic hydrocarbons and the unidentified infrared emission bands - Auto exhaust along the Milky Way

2. Formation of massive stars by growing accretion rate

3. The photoevaporation of interstellar clouds. I - Radiation-driven implosion

4. Catalog of CO radial velocities toward galactic H II regions

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