Zobrazeno 1 - 10
of 89
pro vyhledávání: '"Woods, T. E."'
Autor:
Safi-Harb, S., Burdge, K. B., Bodaghee, A., An, H., Guest, B., Hare, J., Hebbar, P., Ho, W. C. G., Kargaltsev, O., Kirmizibayrak, D., Klingler, N., Nynka, M., Reynolds, M. T., Sasaki, M., Sridhar, N., Vasilopoulos, G., Woods, T. E., Yang, H., Heinke, C., Kong, A., Li, J., MacMaster, A., Mallick, L., Treyturik, C., Tsuji, N., Binder, B., Braun, C., Chang, H. -K., Chatterjee, A., Ferrand, G., Holland-Ashford, T., Ng, C. -Y., Plotkin, R., Romani, R., Zhang, S.
Compact objects and supernova remnants provide nearby laboratories to probe the fate of stars after they die, and the way they impact, and are impacted by, their surrounding medium. The past five decades have significantly advanced our understanding
Externí odkaz:
http://arxiv.org/abs/2311.07673
Symbiotic binaries are long period interacting binaries consisting of a white dwarf (WD) accreting material from a cool evolved giant star via stellar winds. In this paper we study the symbiotic binary LIN 358 located in the SMC. We have observed LIN
Externí odkaz:
http://arxiv.org/abs/2011.02864
Supersoft X-ray sources (SSS) have been identified as white dwarfs accreting from binary companions and undergoing nuclear-burning of the accreted material on their surface. Although expected to be a relatively numerous population from both binary ev
Externí odkaz:
http://arxiv.org/abs/2009.09403
Autor:
Goodwin, A. J., Woods, T. E.
Observations of the accretion powered millisecond pulsar SAX J1808.4-3658 have revealed an interesting binary evolution, with the orbit of the system expanding at an accelerated rate. We use the recent finding that the accreted fuel in SAX J1808.4-36
Externí odkaz:
http://arxiv.org/abs/2003.02970
Autor:
Woods, T. E., Alexandroff, R. M., Ellison, S. L., Ferrarese, L., Gallagher, S. C., Gallo, L., Haggard, D., Hall, P. B., Hlavacek-Larrondo, J., Khatu, V. C., Man, A. W. S., McGee, S., McNamara, B. R., Ruan, J., Sivakoff, G., Stairs, I. H., Willott, C.
The next generation of electromagnetic and gravitational wave observatories will open unprecedented windows to the birth of the first supermassive black holes. This has the potential to reveal their origin and growth in the first billion years, as we
Externí odkaz:
http://arxiv.org/abs/1910.06346
Major mergers of gas-rich galaxies provide promising conditions for the formation of supermassive black holes (SMBHs; $\gtrsim10^5$ M$_\odot$) by direct collapse because they can trigger mass inflows as high as $10^4-10^5$ M$_\odot$ yr$^{-1}$ on sub-
Externí odkaz:
http://arxiv.org/abs/1910.04776
Autor:
Chen, Hai-Liang, Woods, T. E., Yungelson, L. R., Piersanti, Luciano, Gilfanov, M., Han, Zhanwen
Novae are the observational manifestations of thermonuclear runaways on the surface of accreting white dwarfs (WDs). Although novae are an ubiquitous phenomenon, their properties at low metallicity are not well understood. Using the publicly-availabl
Externí odkaz:
http://arxiv.org/abs/1909.07643
Type Ia supernovae are vital to our understanding of the Universe due to their use in measuring cosmological distances and their significance in enriching the interstellar medium with heavy elements. They are understood to be the thermonuclear explos
Externí odkaz:
http://arxiv.org/abs/1812.08799
The evolutionary mechanism underlying Type Ia supernova explosions remains unknown. Recent efforts to constrain progenitor models based on the influence that their high energy emission would have on the interstellar medium (ISM) of galaxies have prov
Externí odkaz:
http://arxiv.org/abs/1807.03798
Publikováno v:
Nature Astronomy (2017)
Type Ia supernovae have proven vital to our understanding of cosmology, both as standard candles and for their role in galactic chemical evolution; however, their origin remains uncertain. The canonical accretion model implies a hot and luminous prog
Externí odkaz:
http://arxiv.org/abs/1709.09190