The Daily Brew
Selected astro-ph abstracts for Thursday 2016 August 18
- Response of the Milky Way's disc to the Large Magellanic Cloud in a first infall scenario
Chervin F. P. Laporte, Facundo A. Gómez, Gurtina Besla, Kathryn V. Johnston, Nicolas Garavito-Camargo
[ arXiv:1608.04743v1 | PDF File ]
- Laboratory measurements compellingly support charge-exchange mechanism for the 'dark matter' $\sim$3.5 keV X-ray line
Chintan Shah (1), Stepan Dobrodey (1), Sven Bernitt (1 and 2), René Steinbrügge (1), José R. Crespo López-Urrutia (1), Liyi Gu (3), Jelle Kaastra (3 and 4) ((1) Max-Planck-Institut für Kernphysik, (2) Institut für Optik und Quantenelektronik, Friedrich-Schiller-Universität, (3) SRON Netherlands Institute for Space Research, Sorbonnelaan 2, (4) Leiden Observatory, Leiden University)
[ arXiv:1608.04751v1 | PDF File ]
- The awakening of a classical nova from hibernation
P. Mroz, A. Udalski, P. Pietrukowicz, M.K. Szymanski, I. Soszynski, L. Wyrzykowski, R. Poleski, S. Kozlowski, J. Skowron, K. Ulaczyk, D. Skowron, M. Pawlak
[ arXiv:1608.04753v1 | PDF File ]
- Modelling Dust Evolution in Galaxies with a Multiphase, Inhomogeneous ISM
Svitlana Zhukovska, Clare Dobbs, Edward B. Jenkins, Ralf Klessen
[ arXiv:1608.04781v1 | PDF File ]
- Portrait of a dark horse: photometric properties and kinematics of the ultra-faint Milky Way satellite Pegasus III
Dongwon Kim, Helmut Jerjen, Marla Geha, Anirudh Chiti, Antonino P. Milone, Dougal Mackey, Gary Da Costa, Anna Frebel, Blair Conn
[ arXiv:1608.04934v1 | PDF File ]
- Sloan Great Wall as a complex of superclusters with collapsing cores
Maret Einasto, Heidi Lietzen, Mirt Gramann, Elmo Tempel, Enn Saar, Lauri Juhan Liivamägi, Pekka Heinämäki, Pasi Nurmi, Jaan Einasto
[ arXiv:1608.04988v1 | PDF File ]
- Ice Grain Collisions in Comparison: CO$_2$, H$_2$O and their Mixtures
Grzegorz Musiolik, Jens Teiser, Tim Jankowski, Gerhard Wurm
[ arXiv:1608.05017v1 | PDF File ]
Other Papers:
- Numerical Simulations of Turbulent, Molecular Clouds Regulated by
Radiation Feedback Forces I: Star Formation Rate and Efficiency
arXiv:1608.04469
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