Zobrazeno 1 - 10
of 26
pro vyhledávání: '"Murray, Norman W."'
Autor:
Li, Yuan, Gendron-Marsolais, Marie-Lou, Zhuravleva, Irina, Xu, Siyao, Simionescu, Aurora, Tremblay, Grant R., Lochhaas, Cassandra, Bryan, Greg L., Quataert, Eliot, Murray, Norman W., Boselli, Alessandro, Hlavacek-Larrondo, Julie, Zheng, Yong, Fossati, Matteo, Li, Miao, Emsellem, Eric, Sarzi, Marc, Arzamasskiy, Lev, Vishniac, Ethan T.
Supermassive black holes (SMBHs) are thought to provide energy that prevents catastrophic cooling in the centers of massive galaxies and galaxy clusters. However, it remains unclear how this "feedback" process operates. We use high-resolution optical
Externí odkaz:
http://arxiv.org/abs/1911.06329
Publikováno v:
Phys. Rev. D 94, 023001 (2016)
Direct detection of black hole-neutron star pairs is anticipated with the advent of aLIGO. Electromagnetic counterparts may be crucial for a confident gravitational-wave detection as well as for extraction of astronomical information. Yet black hole-
Externí odkaz:
http://arxiv.org/abs/1601.00017
Motivated by the nonlinear star formation efficiency found in recent numerical simulations by a number of workers, we perform high-resolution adaptive mesh refinement simulations of star formation in self-gravitating turbulently driven gas. As we fol
Externí odkaz:
http://arxiv.org/abs/1509.05910
Autor:
Murray, Norman W., Chang, Philip
We present a model of star formation in self-gravitating turbulent gas. We treat the turbulent velocity $v_T$ as a dynamical variable, and assume that it is adiabatically heated by the collapse. The theory predicts the run of density, infall velocity
Externí odkaz:
http://arxiv.org/abs/1407.6373
Radial velocity surveys find Jupiter mass planets with semi-major axes a less than 0.1 AU around ~1% of solar-type stars; counting planets with $a$ as large as 5 AU, the fraction of stars having planets reaches ~ 10% {Marcy,Butler}. An examination of
Externí odkaz:
http://arxiv.org/abs/0706.0732
Autor:
Holman, Matthew J., Murray, Norman W.
Publikováno v:
Science 307:1288-1291,2005
Future surveys for transiting extrasolar planets, including the space-based mission Kepler (Borucki et al 2003), are expected to detect hundreds of Jovian mass planets and tens of terrestrial mass planets. For many of these newly discovered planets,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412028
Autor:
Holman, Matthew J., Murray, Norman W.
Publikováno v:
Science, 2005 Feb . 307(5713), 1288-1291.
Externí odkaz:
https://www.jstor.org/stable/3840219
Akademický článek
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Autor:
Murray, Norman W.
Publikováno v:
Science, 2012 Jun 01. 336(6085), 1121-1122.
Externí odkaz:
http://dx.doi.org/10.1126/science.1222590
Akademický článek
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