Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Zongnan Li"'
Autor:
Christopher J. R. Clark, Walter Kieran Gear, Sarah Ragan, Pauline Barmby, Gayathri Athikkat-Eknath, Scott Chapman, Mark G. Rawlings, Matthew W. L. Smith, En-Tzu Lin, Xindi Tang, Francisca Kemper, Thomas G. Williams, Haley Louise Gomez, Sihan Jiao, Zongnan Li, Ilse De Looze, Eun Jung Chung, Brian Cho, Jinhua He, Junfeng Wang, C. D. Wilson, Richard de Grijs, Dimitra Rigopoulou, Anthony Peter Whitworth, Albert K. H. Kong, David L. Clements, Eric W. Koch, Hui-Hsuan Chung, Luis C. Ho, Kate Pattle, Steve Mairs, Chien-Hsiu Lee, Andreas Schruba, Martin Bureau, G. P. Ford, Stephen Anthony Eales, T. M. Hughes, Bumhyun Lee, Aeree Chung, Michał J. Michałowski, Timothy A. Davis, Yingjie Peng, David Eden, Amélie Saintonge, Ming Zhu, Florian Kirchschlager, Yu Gao, Kijeong Yim, Zhiyuan Li
Publikováno v:
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
The Astrophysical Journal Supplement Series
Physics and Astronomy Publications
Astrophysical Journal Supplement Series
The Astrophysical Journal Supplement Series
Physics and Astronomy Publications
Astrophysical Journal Supplement Series
Observing nearby galaxies with submillimeter telescopes on the ground has two major challenges. First, the brightness is significantly reduced at long submillimeter wavelengths compared to the brightness at the peak of the dust emission. Second, it i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2bf10b2300c8a9397569ba9ac619bb3e
https://hdl.handle.net/1854/LU-8745310
https://hdl.handle.net/1854/LU-8745310
Quenched massive spiral galaxies have attracted great attention recently, as more data is available to constrain their environment and cold gas content. However, the quenching mechanism is still uncertain, as it depends on the mass range and baryon b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4516a5a6928e16fee80bf78b2ba8bf94
Publikováno v:
The Astrophysical Journal Supplement Series. 122:257-268
This is the second paper of our spectroscopic confirmation of 55 CV candidates listed in the Downes et al. catalog of cataclysmic variables. Twenty-seven confirmed CVs have been published in the first paper in this series. In this paper we present lo