Physical properties of the fullerene C60-containing planetary nebula SaSt2-3★-Reference-Cited by-同舟云学术

Physical properties of the fullerene C60-containing planetary nebula SaSt2-3★

Published:2018-10-23 Issue:2 Volume:482 Page:2354-2373
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Otsuka Masaaki¹²^ORCID

Affiliation:

1. Okayama Observatory, Kyoto University, Kamogata, Asakuchi, Okayama 719-0232, Japan

2. Academia Sinica, Institute of Astronomy and Astrophysics, 11F Astronomy-Mathematics Building, NTU/AS campus, No. 1, Section 4, Roosevelt Rd., Taipei 10617, Taiwan, Republic of China

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/482/2/2354/26576095/sty2733.pdf

Reference79 articles.

1. ON THE EXCITATION AND FORMATION OF CIRCUMSTELLAR FULLERENES

2. Formation of buckminsterfullerene (C60) in interstellar space

3. Top-down formation of fullerenes in the interstellar medium

4. Atmospheric extinction properties above Mauna Kea from the Nearby SuperNova Factory spectro-photometric data set

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