A newly identified emission-line region around P Cygni-Reference-Cited by-同舟云学术

A newly identified emission-line region around P Cygni

Published:2018-08-18 Issue:1 Volume:481 Page:793-805
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Mizumoto Misaki¹²,Kobayashi Naoto³⁴⁵,Hamano Satoshi⁵,Ikeda Yuji⁵⁶,Kondo Sohei⁵,Sameshima Hiroaki⁵,Matsunaga Noriyuki¹⁵,Fukue Kei⁵,Yasui Chikako⁷,Izumi Natsuko⁷,Kawakita Hideyo⁵⁸,Nakanishi Kenshi⁵⁸,Nakaoka Tetsuya⁵⁸,Otsubo Shogo⁵⁸,Maehara Hiroyuki⁹

Affiliation:

1. Department of Astronomy, Graduate School of Science, The University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan

2. Centre for Extragalactic Astronomy, Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK

3. Kiso Observatory, Institute of Astronomy, School of Science, The University of Tokyo, Mitake, Kiso-machi, Kiso-gun, Nagano 397-0101, Japan

4. Institute of Astronomy, Graduate School of Science, The University of Tokyo, Osawa, Mitaka, Tokyo 181-0015, Japan

5. Laboratory of IR High-resolution Spectroscopy (LIH), Koyama Astronomical Observatory, Kyoto Sangyo University, Motoyama, Kamigamo, Kita-Ku, Kyoto 603-8555, Japan

6. Photocoding, Iwakura-Kita-Ikedacho, Sakyo-Ku, Kyoto 606-0004, Japan

7. National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588, Japan

8. Department of Physics, Faculty of Science, Kyoto Sangyo University, Motoyama, Kamigamo, Kita-ku, Kyoto 603-8555, Japan

9. Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Honjo, Kamogata, Asakuchi, Okayama 719-0232, Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/481/1/793/25697570/sty2239.pdf

Reference52 articles.

1. A high-resolution image of the inner shell of the P Cygni nebula in the infrared [Fe ii] line

2. PENETRATING THE HOMUNCULUS—NEAR-INFRARED ADAPTIVE OPTICS IMAGES OF ETA CARINAE

3. The shock-excited P Cygni nebula

4. Adaptive optics imaging of P Cygni in H$_{\alpha}$

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