FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). III. Possible evidence for formation of NGC 6618 cluster in M 17 by cloud

FOREST Unbiased Galactic plane Imaging survey with the Nobeyama 45 m telescope (FUGIN). III. Possible evidence for formation of NGC 6618 cluster in M 17 by cloud–cloud collision

Published:2018-03-01 Issue:SP2 Volume:70 Page:
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:

Author:

Nishimura Atsushi¹,Minamidani Tetsuhiro²³,Umemoto Tomofumi²³,Fujita Shinji¹,Matsuo Mitsuhiro²,Hattori Yusuke¹,Kohno Mikito¹,Yamagishi Mitsuyoshi⁴,Tsuda Yuya⁵,Kuriki Mika⁶,Kuno Nario⁶⁷,Torii Kazufumi²³,Tsutsumi Daichi¹,Okawa Kazuki¹,Sano Hidetoshi¹⁸,Tachihara Kengo¹,Ohama Akio¹,Fukui Yasuo¹⁸

Affiliation:

1. Department of Physics, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan

2. Nobeyama Radio Observatory, National Astronomical Observatory of Japan (NAOJ), National Institutes of Natural Sciences (NINS), 462-2 Nobeyama, Minamimaki, Minamisaku, Nagano 384-1305, Japan

3. Department of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan

4. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Chuo-ku, Sagamihara, Kanagawa 252-5210, Japan

5. Graduate School of Science and Engineering, Meisei University, 2-1-1 Hodokubo, Hino, Tokyo 191-0042, Japan

6. Department of Physics, University of Tsukuba, 1-1-1 Ten-nodai, Tsukuba, Ibaraki 305-8577, Japan

7. Tomonaga Center for the History of the Universe, University of Tsukuba, 1-1-1 Tennodai, Tsukuba, Ibaraki 305-8571, Japan

8. Institute for Advanced Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8601, Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/70/SP2/S42/24971937/psx149.pdf

Reference120 articles.

1. Supersonic cloud collision. I.

2. Supersonic cloud collision – II

3. Astropy: A community Python package for astronomy

4. Star formation triggered by non-head-on cloud–cloud collisions, and clouds with pre-collision sub-structure

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