scholarly journals Erratum: Molecular clouds in the NGC 6334 and NGC 6357 region: Evidence for a 100 pc–scale cloud–cloud collision triggering the Galactic mini-starbursts

2018 ◽  
Vol 70 (SP2) ◽  
Author(s):  
Yasuo Fukui ◽  
Mikito Kohno ◽  
Keiko Yokoyama ◽  
Kazufumi Torii ◽  
Yusuke Hattori ◽  
...  
Keyword(s):  
Molecular Clouds ◽  
Ngc 6334

scholarly journals Massive Stars in Molecular Clouds Rich in High-energy Sources: The Bridge of G332.809–0.132 and CS 78 in NGC 6334

2020 ◽  
Vol 160 (2) ◽  
pp. 65 ◽  
Author(s):  
Maria Messineo ◽  
Karl M. Menten ◽  
Donald F. Figer ◽  
J. Simon Clark
Keyword(s):  
Molecular Clouds ◽  
Massive Stars ◽  
High Energy ◽  
Energy Sources ◽  
Ngc 6334

Hard X-ray emission from giant molecular clouds NGC 6334 and M17

1999 ◽  
Vol 320 (4-5) ◽  
pp. 323-323 ◽  
Author(s):  
K. Matsuzaki ◽  
Y. Sekimoto ◽  
T. Kamae ◽  
S. Yamamoto ◽  
K. Tatematsu ◽  
...  
Keyword(s):  
Molecular Clouds ◽  
Giant Molecular Clouds ◽  
X Ray ◽  
Ngc 6334

scholarly journals Molecular clouds in the NGC 6334 and NGC 6357 region: Evidence for a 100 pc-scale cloud–cloud collision triggering the Galactic mini-starbursts

2018 ◽  
Vol 70 (SP2) ◽  
Author(s):  
Yasuo Fukui ◽  
Mikito Kohno ◽  
Keiko Yokoyama ◽  
Kazufumi Torii ◽  
Yusuke Hattori ◽  
...  
Keyword(s):  
Molecular Clouds ◽  
Ngc 6334

Formation of the twin galactic starburst regions NGC 6357 and NGC 6334

2015 ◽  
Vol 12 (S316) ◽  
pp. 173-174
Author(s):  
Kazufumi Torii ◽  
Keisuke Hasegawa ◽  
Akio Ohama ◽  
Hiroaki Yamamoto ◽  
Kengo Tachihara ◽  
...  
Keyword(s):  
Star Formation ◽  
Molecular Clouds ◽  
Relative Velocity ◽  
High Mass ◽  
Mass Star ◽  
Ngc 6334 ◽  
Starburst Regions

AbstractNew CO J=1–0 observations with NANTEN and NANTEN2 reveal that extensive collisions between two molecular clouds at relative velocity of 15 km s−1 triggered the O star formation in the Galactic mini-starbursts NGC 6357 and NGC 6334. Correlated/anti-correlated gas distributions and intermediate velocity features between the two clouds lend support for the cloud-cloud collision scenario. The timescale of the collision and high-mass star formation is as short as less than 0.5 Myrs, suggesting rapid O star formation.

Angular size of OH emission regions

1967 ◽  
Vol 31 ◽  
pp. 71-72
Author(s):  
B. F. Burke ◽  
P. P. Crowther ◽  
J. M. Moran ◽  
A. E. E. Rogers ◽  
J. A. Ball ◽  
...  
Keyword(s):  
Angular Size ◽  
Emission Sources ◽  
Ngc 6334

Interferometry gives effective diameters less than 20″ for the OH emission sources in W3and Sgr B2. The sources in W49and NGC 6334 contain two or more components, some of which are smaller than 25″.

Structure of the turbulent atomic gas and formation of molecular clouds

2008 ◽  
Vol 31 ◽  
pp. 15-18
Author(s):  
P. Hennebelle ◽  
E. Audit
Keyword(s):  
Molecular Clouds ◽  
Atomic Gas
Sign in / Sign up

Export Citation Format

Share Document