The Daily Brew
Selected astro-ph abstracts for Wednesday 2015 August 26
- Deep Chandra, HST-COS, and Megacam Observations of the Phoenix Cluster: Extreme Star Formation and AGN Feedback on Hundred Kiloparsec Scales
M. McDonald, B. R. McNamara, R. J. van Weeren, D. E. Applegate, M. Bayliss, M. W. Bautz, B. A. Benson, J. E. Carlstrom, L. E. Bleem, M. Chatzikos, A. C. Edge, A. C. Fabian, G. P. Garmire, J. Hlavacek-Larrondo, C. Jones-Forman, A. B. Mantz, E. D. Miller, B. Stalder, S. Veilleux, J. A. Zuhone
[ arXiv:1508.05941v1 | PDF File ]
- ALMA Observations of the Active Nucleus of NGC 7469
Takuma Izumi, Kotaro Kohno, Susanne Aalto, Akihiro Doi, Daniel Espada, Kambiz Fathi, Nanase Harada, Bunyo Hatsukade, Takashi Hattori, Pei-Ying Hsieh, Soh Ikarashi, Masatoshi Imanishi, Daisuke Iono, Sumio Ishizuki, Melanie Krips, Sergio Martín, Satoki Matsushita, David S. Meier, Hiroshi Nagai, Naomasa Nakai, Taku Nakajima, Kouichiro Nakanishi, Hideko Nomura, Michael W. Regan, Eva Schinnerer, Kartik Sheth, Shuro Takano, Yoichi Tamura, Yuichi Terashima, Tomoka Tosaki, Jean L. Turner, Hideki Umehata, Tommy Wiklind
[ arXiv:1508.05946v1 | PDF File ]
- SXDF-ALMA 1.5 arcmin^2 deep survey. A compact dusty star-forming galaxy at z=2.5
Ken-ichi Tadaki, Kotaro Kohno, Tadayuki Kodama, Soh Ikarashi, Itziar Aretxaga, Stefano Berta, Karina I. Caputi, James S. Dunlop, Bunyo Hatsukade, Masao Hayashi, David H. Hughes, Rob Ivison, Takuma Izumi, Yusei Koyama, Dieter Lutz, Ryu Makiya, Yuichi Matsuda, Kouichiro Nakanishi, Wiphu Rujopakarn, Yoichi Tamura, Hideki Umehata, Wei-Hao Wang, Grant W. Wilson, Stijn Wuyts, Yuki Yamaguchi, Min S. Yun
[ arXiv:1508.05950v1 | PDF File ]
- A self-consistent, absolute isochronal age scale for young moving groups in the solar neighbourhood
Cameron P. M. Bell (1), Eric E. Mamajek (1), Tim Naylor (2) ((1) University of Rochester, (2) University of Exeter)
[ arXiv:1508.05955v1 | PDF File ]
- On Measuring the Metallicity of Supernovae Type Ia Progenitors
Broxton J. Miles, Daniel R. van Rossum, Dean M. Townsley, F. X. Timmes, Aaron P. Jackson, Alan C. Calder, Edward F. Brown
[ arXiv:1508.05961v1 | PDF File ]
- What drives the M*-SFR relation turning over at high masses? The role of bulges
Zhizheng Pan, Xianzhong Zheng, Weipeng Lin, Jinrong Li, Jing Wang, Lulu Fan, Xu Kong
[ arXiv:1508.06017v1 | PDF File ]
- Globular cluster formation efficiencies from black-hole X-ray binary feedback
Stephen Justham, Eric W. Peng, Kevin Schawinski
[ arXiv:1508.06046v1 | PDF File ]
- The modelling of feedback in star formation simulations
James E. Dale
[ arXiv:1508.06054v1 | PDF File ]
- Empirical metallicity-dependent calibrations of effective temperature against colours for dwarfs and giants based on interferometric data
Yang Huang (Peking University), Xiao-Wei Liu, Hai-Bo Yuan, Mao-sheng Xiang, Bing-Qiu Chen, Hua-Wei Zhang
[ arXiv:1508.06080v1 | PDF File ]
- Supernova SN 1006 in two historic Yemeni reports
Wafiq Rada (Hilla University College, Babylon, Iraq), Ralph Neuhaeuser (U Jena)
[ arXiv:1508.06126v1 | PDF File ]
- Preserving chemical signatures of primordial star formation in the first low-mass stars
Alexander P. Ji (MIT), Anna Frebel (MIT), Volker Bromm (UT Austin)
[ arXiv:1508.06137v1 | PDF File ]
- On the stability of non-isothermal Bonnor-Ebert spheres. II. The effect of gas temperature on the stability
O. Sipilä, J. Harju, M. Juvela
[ arXiv:1508.06151v1 | PDF File ]
- A remarkable recurrent nova in M 31: The 2010 eruption recovered and evidence of a six-month period
M. Henze, M. J. Darnley, F. Kabashima, K. Nishiyama, K. Itagaki, X. Gao
[ arXiv:1508.06205v1 | PDF File ]
Other Papers:
- Testing the origin of ~3.55 keV line in individual galaxy clusters
observed with XMM-Newton
arXiv:1508.05186
- Shock Revival in Core-Collapse Supernovae: A Phase-Diagram Analysis
arXiv:1508.03640
- Early Science with the Large Millimeter Telescope: CO and [C II]
Emission in the z=4.3 AzTEC J095942.9+022938 (COSMOS AzTEC-1)
arXiv:1508.05425
- The Ages of A-Stars I: Interferometric Observations and Age Estimates
for Stars in the Ursa Major Moving Group
arXiv:1508.05643
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