Zobrazeno 1 - 10
of 59
pro vyhledávání: '"Heuvel, E. P. J. Van den"'
Autor:
Marino, A., Yang, H., Zelati, F. Coti, Rea, N., Guillot, S., Jaisawal, G. K., Maitra, C., Ness, J. -U., Haberl, F., Kuulkers, E., Yuan, W., Feng, H., Tao, L., Jin, C., Sun, H., Zhang, W., Chen, W., Heuvel, E. P. J. van den, Soria, R., Zhang, B., Weng, S. -S., Ji, L., Zhang, G. B., Pan, X., Lv, Z., Zhang, C., Ling, Z., Chen, Y., Jia, S., Liu, Y., Cheng, H. Q., Li, D. Y., Gendreau, K. C., Ng, M., Strohmayer, T. E.
On May 27 2024, the Wide-field X-ray Telescope onboard the Einstein Probe (EP) mission detected enhanced X-ray emission from a new transient source in the Small Magellanic Cloud (SMC) during its commissioning phase. Prompt follow-up with the EP Follo
Externí odkaz:
http://arxiv.org/abs/2407.21371
We report the observation of a possible optical counterpart to the recently discovered X-ray source NuSTAR J053449+2126.0 (J0534 in short). We observed the source location using the 1.5-m Telescope (RTT150) to search for an optical counterpart, and d
Externí odkaz:
http://arxiv.org/abs/2302.08994
Publikováno v:
A&A 636, A99 (2020)
Theoretical population number studies of binaries with at least one black hole (BH) component are obviously depending on whether or not BHs receive a (natal) kick during their formation. Several observational facts seem to indicate that indeed BHs re
Externí odkaz:
http://arxiv.org/abs/1912.01256
Autor:
Belczynski, K., Bulik, T., Olejak, A., Chruslinska, M., Singh, N., Pol, N., Zdunik, L., O'Shaughnessy, R., McLaughlin, M., Lorimer, D., Korobkin, O., Heuvel, E. P. J. van den, Davies, M. B., Holz, D. E.
The first neutron star-neutron star merger was detected in by LIGO/Virgo in a galaxy in which the majority of star formation was taking place a long time ago (11 Gyr). LIGO/Virgo estimated that local cosmic NS-NS merger rate is 110-3840 Gpc^-3 yr^-1.
Externí odkaz:
http://arxiv.org/abs/1812.10065
Autor:
Tauris, T. M., Kramer, M., Freire, P. C. C., Wex, N., Janka, H. -T., Langer, N., Podsiadlowski, Ph., Bozzo, E., Chaty, S., Kruckow, M. U., Heuvel, E. P. J. van den, Antoniadis, J., Breton, R. P., Champion, D. J.
Publikováno v:
The Astrophysical Journal, 846, 170 (2017)
Double neutron star (DNS) systems represent extreme physical objects and the endpoint of an exotic journey of stellar evolution and binary interactions. Large numbers of DNS systems and their mergers are anticipated to be discovered using the Square-
Externí odkaz:
http://arxiv.org/abs/1706.09438
Autor:
Ivanova, N., Justham, S., Chen, X., De Marco, O., Fryer, C. L., Gaburov, E., Ge, H., Glebbeek, E., Han, Z., Li, X. -D., Lu, G., Marsh, T., Podsiadlowski, Ph., Potter, A., Soker, N., Taam, R., Tauris, T. M., Heuvel, E. P. J. van den, Webbink, R. F.
This work aims to present our current best physical understanding of common-envelope evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas which should point the way forward for progress in this important but long-standi
Externí odkaz:
http://arxiv.org/abs/1209.4302
Autor:
Liu, X. W., Xu, R. X., Heuvel, E. P. J. van den, Qiao, G. J., Han, J. L., Han, Z. W., Li, X. D.
Publikováno v:
2015ApJ...799..233L
The origin of the 6.67 hr period X-ray source, 1E161348-5055, in the young supernova remnant RCW 103 is puzzling. We propose that it may be the descendant of a Thorne-Zytkow Object (TZO). A TZO may at its formation have a rapidly spinning neutron sta
Externí odkaz:
http://arxiv.org/abs/1207.4687
Autor:
Kuulkers, E., Kouveliotou, C., Belloni, T., Bel, M. Cadolle, Chenevez, J., Trigo, M. Diaz, Homan, J., Ibarra, A., Kennea, J. A., Munoz-Darias, T., Ness, J. -U., Parmar, A. N., Pollock, A. M. T., Heuvel, E. P. J. van den, van der Horst, A. J.
MAXI J1659-152 is a bright X-ray transient black-hole candidate binary system discovered in September 2010. We report here on MAXI, RXTE, Swift, and XMM-Newton observations during its 2010/2011 outburst. We find that during the first one and a half w
Externí odkaz:
http://arxiv.org/abs/1204.5840
The low mass X-ray binary (LMXB) IGR J17480-2446 in the globular cluster Terzan 5 harbors an 11 Hz accreting pulsar. This is the first object discovered in a globular cluster with a pulsar spinning at such low rate. The accreting pulsar is anomalous
Externí odkaz:
http://arxiv.org/abs/1112.5315
We study mass transfer by Roche lobe overflow in close-in exoplanetary systems. The planet's atmospheric gas passes through the inner Lagrangian point and flows along a narrow stream, accelerating to 100-$200\kms$ velocity before forming an accretion
Externí odkaz:
http://arxiv.org/abs/1005.4497