%0 Generic %1 citeulike:13815401 %A Miller, Jon M. %A Kaastra, Jelle S. %A Miller, M. Coleman %A Reynolds, Mark T. %A Brown, Gregory %A Cenko, S. Bradley %A Drake, Jeremy J. %A Gezari, Suvi %A Guillochon, James %A Gultekin, Kayhan %A Irwin, Jimmy %A Levan, Andrew %A Maitra, Dipankar %A Maksym, W. Peter %A Mushotzky, Richard %A O'Brien, Paul %A Paerels, Frits %A de Plaa, Jelle %A Ramirez-Ruiz, Enrico %A Strohmayer, Tod %A Tanvir, Nial %D 2015 %K imported %T Flows of X-ray gas reveal the disruption of a star by a massive black hole %U http://arxiv.org/abs/1510.06348 %X Tidal forces close to massive black holes can violently disrupt stars that make a close approach. These extreme events are discovered via bright X-ray and optical/UV flares in galactic centers. Prior studies based on modeling decaying flux trends have been able to estimate broad properties, such as the mass accretion rate. Here we report the detection of flows of highly ionized X-ray gas in high-resolution X-ray spectra of a nearby tidal disruption event. Variability within the absorption-dominated spectra indicates that the gas is relatively close to the black hole. Narrow line widths indicate that the gas does not stretch over a large range of radii, giving a low volume filling factor. Modest outflow speeds of a few hundred kilometers per second are observed, significantly below the escape speed from the radius set by variability. The gas flow is consistent with a rotating wind from the inner, super-Eddington region of a nascent accretion disk, or with a filament of disrupted stellar gas near to the apocenter of an elliptical orbit. Flows of this sort are predicted by fundamental analytical theory and more recent numerical simulations.

@misc{citeulike:13815401, abstract = {{Tidal forces close to massive black holes can violently disrupt stars that make a close approach. These extreme events are discovered via bright X-ray and optical/UV flares in galactic centers. Prior studies based on modeling decaying flux trends have been able to estimate broad properties, such as the mass accretion rate. Here we report the detection of flows of highly ionized X-ray gas in high-resolution X-ray spectra of a nearby tidal disruption event. Variability within the absorption-dominated spectra indicates that the gas is relatively close to the black hole. Narrow line widths indicate that the gas does not stretch over a large range of radii, giving a low volume filling factor. Modest outflow speeds of a few hundred kilometers per second are observed, significantly below the escape speed from the radius set by variability. The gas flow is consistent with a rotating wind from the inner, super-Eddington region of a nascent accretion disk, or with a filament of disrupted stellar gas near to the apocenter of an elliptical orbit. Flows of this sort are predicted by fundamental analytical theory and more recent numerical simulations.}}, added-at = {2019-03-25T08:20:55.000+0100}, archiveprefix = {arXiv}, author = {Miller, Jon M. and Kaastra, Jelle S. and Miller, M. Coleman and Reynolds, Mark T. and Brown, Gregory and Cenko, S. Bradley and Drake, Jeremy J. and Gezari, Suvi and Guillochon, James and Gultekin, Kayhan and Irwin, Jimmy and Levan, Andrew and Maitra, Dipankar and Maksym, W. Peter and Mushotzky, Richard and O'Brien, Paul and Paerels, Frits and de Plaa, Jelle and Ramirez-Ruiz, Enrico and Strohmayer, Tod and Tanvir, Nial}, biburl = {https://www.bibsonomy.org/bibtex/2464dd071f28329e2473ac8527fbcf979/ericblackman}, citeulike-article-id = {13815401}, citeulike-linkout-0 = {http://arxiv.org/abs/1510.06348}, citeulike-linkout-1 = {http://arxiv.org/pdf/1510.06348}, day = 21, eprint = {1510.06348}, interhash = {53349151be0a644c8132703f738df327}, intrahash = {464dd071f28329e2473ac8527fbcf979}, keywords = {imported}, month = oct, posted-at = {2015-10-28 08:10:29}, priority = {2}, timestamp = {2019-03-25T08:20:55.000+0100}, title = {{Flows of X-ray gas reveal the disruption of a star by a massive black hole}}, url = {http://arxiv.org/abs/1510.06348}, year = 2015 }