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• W4285403750 endingPage "203" @default.
• W4285403750 startingPage "203" @default.
• W4285403750 abstract "Recent analyses have shown that close encounters between stars and stellar black holes occur frequently in dense star clusters. Depending upon the distance at closest approach, these interactions can lead to dissipating encounters such as tidal captures and disruptions, or direct physical collisions, all of which may be accompanied by bright electromagnetic transients. In this study, we perform a wide range of hydrodynamic simulations of close encounters between black holes and main-sequence stars that collectively cover the parameter space of interest, and we identify and classify the various possible outcomes. In the case of nearly head-on collisions, the star is completely disrupted with roughly half of the stellar material becoming bound to the black hole. For more distant encounters near the classical tidal-disruption radius, the star is only partially disrupted on the first pericenter passage. Depending upon the interaction details, the partially disrupted stellar remnant may be tidally captured by the black hole or become unbound (in some cases, receiving a sufficiently large impulsive kick from asymmetric mass loss to be ejected from its host cluster). In the former case, the star will undergo additional pericenter passages before ultimately being disrupted fully. Based on the properties of the material bound to the black hole at the end of our simulations (in particular, the total bound mass and angular momentum), we comment upon the expected accretion process and associated electromagnetic signatures that are likely to result." @default.
• W4285403750 created "2022-07-14" @default.
• W4285403750 creator A5037828745 @default.
• W4285403750 creator A5045415901 @default.
• W4285403750 creator A5050742735 @default.
• W4285403750 creator A5068003012 @default.
• W4285403750 creator A5080898367 @default.
• W4285403750 date "2022-07-01" @default.
• W4285403750 modified "2023-10-06" @default.
• W4285403750 title "Hydrodynamics of Collisions and Close Encounters between Stellar Black Holes and Main-sequence Stars" @default.
• W4285403750 cites W1498822667 @default.
• W4285403750 cites W1533662085 @default.
• W4285403750 cites W1537652385 @default.
• W4285403750 cites W1570143824 @default.
• W4285403750 cites W1775426370 @default.
• W4285403750 cites W1777135035 @default.
• W4285403750 cites W1912595871 @default.
• W4285403750 cites W1965345886 @default.
• W4285403750 cites W1968036988 @default.
• W4285403750 cites W1975112881 @default.
• W4285403750 cites W1977825268 @default.
• W4285403750 cites W1990670404 @default.
• W4285403750 cites W1995032213 @default.
• W4285403750 cites W1998104730 @default.
• W4285403750 cites W2009530585 @default.
• W4285403750 cites W2011022699 @default.
• W4285403750 cites W2014470520 @default.
• W4285403750 cites W2015295900 @default.
• W4285403750 cites W2020203444 @default.
• W4285403750 cites W2027649935 @default.
• W4285403750 cites W2028925143 @default.
• W4285403750 cites W2030304981 @default.
• W4285403750 cites W2030644965 @default.
• W4285403750 cites W2032794526 @default.
• W4285403750 cites W2034961162 @default.
• W4285403750 cites W2038337533 @default.
• W4285403750 cites W2039954136 @default.
• W4285403750 cites W2042547701 @default.
• W4285403750 cites W2045183628 @default.
• W4285403750 cites W2045565446 @default.
• W4285403750 cites W2047244984 @default.
• W4285403750 cites W2049319759 @default.
• W4285403750 cites W2050444942 @default.
• W4285403750 cites W2054901417 @default.
• W4285403750 cites W2055832107 @default.
• W4285403750 cites W2059798232 @default.
• W4285403750 cites W2061151441 @default.
• W4285403750 cites W2061341074 @default.
• W4285403750 cites W2066406099 @default.
• W4285403750 cites W2067029170 @default.
• W4285403750 cites W2070717200 @default.
• W4285403750 cites W2070787987 @default.
• W4285403750 cites W2073799363 @default.
• W4285403750 cites W2074185255 @default.
• W4285403750 cites W2076008831 @default.
• W4285403750 cites W2088308551 @default.
• W4285403750 cites W2097082581 @default.
• W4285403750 cites W2101349161 @default.
• W4285403750 cites W2106325396 @default.
• W4285403750 cites W2109112103 @default.
• W4285403750 cites W2127689830 @default.
• W4285403750 cites W2129760210 @default.
• W4285403750 cites W2131661760 @default.
• W4285403750 cites W2137513434 @default.
• W4285403750 cites W2138040517 @default.
• W4285403750 cites W2203167201 @default.
• W4285403750 cites W2226742632 @default.
• W4285403750 cites W2235109351 @default.
• W4285403750 cites W2254470438 @default.
• W4285403750 cites W2270122817 @default.
• W4285403750 cites W2394580648 @default.
• W4285403750 cites W2482412227 @default.
• W4285403750 cites W2621575995 @default.
• W4285403750 cites W2662353964 @default.
• W4285403750 cites W2755027818 @default.
• W4285403750 cites W2784028283 @default.
• W4285403750 cites W2787299997 @default.
• W4285403750 cites W2902517647 @default.
• W4285403750 cites W2945232811 @default.
• W4285403750 cites W2970187091 @default.
• W4285403750 cites W2989338800 @default.
• W4285403750 cites W2990139692 @default.
• W4285403750 cites W3037378966 @default.
• W4285403750 cites W3039181188 @default.
• W4285403750 cites W3084173438 @default.
• W4285403750 cites W3094847722 @default.
• W4285403750 cites W3098172894 @default.
• W4285403750 cites W3098221464 @default.
• W4285403750 cites W3099885928 @default.
• W4285403750 cites W3099915657 @default.
• W4285403750 cites W3099922616 @default.
• W4285403750 cites W3100343529 @default.
• W4285403750 cites W3100494927 @default.
• W4285403750 cites W3101585058 @default.
• W4285403750 cites W3101788588 @default.
• W4285403750 cites W3102127100 @default.
• W4285403750 cites W3102580607 @default.
• W4285403750 cites W3102725408 @default.

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