Zobrazeno 1 - 10
of 120
pro vyhledávání: '"Rasio, F."'
Autor:
Bailes, M., Barr, E., Bhat, N. D. R., Brink, J., Buchner, S., Burgay, M., Camilo, F., Champion, D. J., Hessels, J., Janssen, G. H., Jameson, A., Johnston, S., Karastergiou, A., Karuppusamy, R., Kaspi, V., Keith, M. J., Kramer, M., McLaughlin, M. A., Moodley, K., Oslowski, S., Possenti, A., Ransom, S. M., Rasio, F. A., Sievers, J., Serylak, M., Stappers, B. W., Stairs, I. H., Theureau, G., van Straten, W., Weltevrede, P., Wex, N.
Publikováno v:
2018, Proceedings of Science, Volume 277, 011, https://pos.sissa.it/277/011/pdf
The MeerKAT telescope represents an outstanding opportunity for radio pulsar timing science with its unique combination of a large collecting area and aperture efficiency (effective area $\sim$7500 m$^2$), system temperature ($T<20$K), high slew spee
Externí odkaz:
http://arxiv.org/abs/1803.07424
We present theoretical models for stellar black hole (BH) properties in young, massive star clusters. Using a Monte Carlo code for stellar dynamics, we model realistic star clusters with $N\simeq 5\times10^5$ stars and significant binary fractions (u
Externí odkaz:
http://arxiv.org/abs/1309.3703
The rapid circularization and synchronization of the stellar components in an eccentric binary system at the onset of Roche lobe overflow (RLO) is a fundamental assumption common to all binary stellar evolution and population synthesis codes, even th
Externí odkaz:
http://arxiv.org/abs/1005.0625
Using our recently improved Monte Carlo evolution code, we study the evolution of the binary fraction in globular clusters. In agreement with previous N-body simulations, we find generally that the hard binary fraction in the core tends to increase w
Externí odkaz:
http://arxiv.org/abs/0907.4196
Publikováno v:
Astrophys.J.702:1387-1392,2009
We investigate the secular evolution of the orbital semi-major axis and eccentricity due to mass transfer in eccentric binaries, allowing for both mass and angular momentum loss from the system. Adopting a delta function mass transfer rate at the per
Externí odkaz:
http://arxiv.org/abs/0903.0621
Autor:
Ghez, A., Morris, M., Lu, J., Weinberg, N., Matthews, K., Alexander, T., Armitage, P., Becklin, E., Brown, W., Campbell, R., Do, T., Eckart, A., Genzel, R., Gould, A., Hansen, B., Ho, L., Lo, F., Loeb, A., Melia, F., Merritt, D., Milosavljevic, M., Perets, H., Rasio, F., Reid, M., Salim, S., Schoedel, R., Yelda, S.
As the closest example of a galactic nucleus, the Galactic center presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environs. Detailed studies of stellar dynamics deep in the potential well of a galaxy, wit
Externí odkaz:
http://arxiv.org/abs/0903.0383
Mergers of double neutron stars are considered the most likely progenitors for short gamma-ray bursts. Indeed such a merger can produce a black hole with a transient accreting torus of nuclear matter (Lee & Ramirez-Ruiz 2007, Oechslin & Janka 2006),
Externí odkaz:
http://arxiv.org/abs/0712.1036
We investigate the secular evolution of the orbital semi-major axis and eccentricity due to mass transfer in eccentric binaries, assuming conservation of total system mass and orbital angular momentum. Assuming a delta function mass transfer rate cen
Externí odkaz:
http://arxiv.org/abs/0706.4312
In this paper, the second of a series, we study the stellar dynamical and evolutionary processes leading to the formation of compact binaries containing neutron stars (NSs) in dense globular clusters (GCs). For this study, 70 dense clusters were simu
Externí odkaz:
http://arxiv.org/abs/0706.4096
Autor:
Willems, B., Kalogera, V., Vecchio, A., Ivanova, N., Rasio, F. A., Fregeau, J. M., Belczynski, K.
We consider the formation of double white dwarfs (DWDs) through dynamical interactions in globular clusters. Such interactions can give rise to eccentric DWDs, in contrast to the exclusively circular population expected to form in the Galactic disk.
Externí odkaz:
http://arxiv.org/abs/0705.4287