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The mass of the central black hole in a galaxy that hosted a tidal disruption event (TDE) is an important parameter in understanding its energetics and dynamics. We present the first homogeneously measured black hole masses of a complete…

The host galaxies of tidal disruption events (TDEs) have been shown to possess peculiar properties, including high central light concentrations, unusual star-formation histories, and ``green'' colors. The ubiquity of these large-scale…

During the tidal disruption of a star by a massive black hole (BH) of mass MBH <~ 10^7 Msun, stellar debris falls back to the BH at a rate well above the Eddington rate. A fraction of this gas is subsequently blown away from the BH,…

宇宙学与河外天体物理 · 物理学 2015-05-19 Linda E. Strubbe , Eliot Quataert

We present the results of X-ray variability and spectral analysis of a sample of 15 new candidates for active galactic nuclei with relatively low-mass black holes (BHs). They are selected from the Second XMM-Newton Serendipitous Source…

高能天体物理现象 · 物理学 2015-06-05 Naoya Kamizasa , Yuichi Terashima , Hisamitsu Awaki

We have measured the stellar velocity dispersions (\sigma_*) and estimated the central black hole (BH) masses for over 900 broad-line active galactic nuclei (AGNs) observed with the Sloan Digital Sky Survey. The sample includes objects…

天体物理学 · 物理学 2009-06-23 J. Shen , D. E. Vanden Berk , D. P. Schneider , P. B. Hall

We have studied the X-ray nuclear activity of 187 nearby (distance < 15 Mpc) galaxies observed with Chandra/ACIS. We found that 86 of them have a point-like X-ray core, consistent with an accreting black hole (BH). We argue that the…

高能天体物理现象 · 物理学 2010-12-02 Wei Ming Zhang , Roberto Soria , Shuang Nan Zhang , Douglas A. Swartz , JiFeng Liu

Liu and collaborators recently proposed an elliptical accretion disk model for tidal disruption events (TDEs). They showed that the accretion disks of optical/UV TDEs are large and highly eccentric and suggested that the broad optical…

高能天体物理现象 · 物理学 2021-02-10 Z. Q. Zhou , F. K. Liu , S. Komossa , R. Cao , L. C. Ho , Xian Chen , Shuo Li

Tidal disruption events (TDEs) provide a means to probe the low end of the supermassive black hole (SMBH) mass distribution, as they are only observable below the Hills mass ($\lesssim 10^8$ M$_\odot$). Here we attempt to calibrate the…

高能天体物理现象 · 物理学 2022-08-16 Paige Ramsden , Daniel Lanning , Matt Nicholl , Sean L. McGee

We present a sample of hard X-ray selected candidate black holes (BHs) in 19 dwarf galaxies. BH candidates are identified by cross-matching a parent sample of ~44,000 local dwarf galaxies (M_stellar < 3 x 10^9 Msun, z<0.055) with the…

星系天体物理 · 物理学 2015-05-27 Sean Lemons , Amy Reines , Richard Plotkin , Elena Gallo , Jenny Greene

We study the properties of tidal disruption event (TDE) host galaxies in the context of a catalog of ~500,000 galaxies from the Sloan Digital Sky Survey. We explore whether selection effects can account for the overrepresentation of TDEs in…

高能天体物理现象 · 物理学 2017-11-16 Jamie Law-Smith , Enrico Ramirez-Ruiz , Sara L. Ellison , Ryan J. Foley

The rate of tidal disruption events (TDEs), $R_\text{TDE}$, is predicted to depend on stellar conditions near the super-massive black hole (SMBH), which are on difficult-to-measure sub-parsec scales. We test whether $R_\text{TDE}$ depends…

高能天体物理现象 · 物理学 2018-02-07 Or Graur , K. Decker French , H. Jabran Zahid , James Guillochon , Kaisey S. Mandel , Katie Auchettl , Ann I. Zabludoff

Using $I$-band images of 35 nearby ($z<0.1$) type 1 active galactic nuclei (AGNs) obtained with Hubble Space Telescope, selected from the 70-month Swift-BAT X-ray source catalog, we investigate the photometric properties of the host…

星系天体物理 · 物理学 2022-05-25 Suyeon Son , Minjin Kim , Aaron J. Barth , Luis C. Ho

We present an expanded sample of low-mass black holes (BHs) found in galactic nuclei. Using standard virial mass techniques to estimate BH masses, we select from the Fourth Data Release of the Sloan Digital Sky Survey all broad-line active…

天体物理学 · 物理学 2009-11-13 Jenny E. Greene , Luis C. Ho

We compare the host galaxies properties of BL Lac objects with those of radio loud quasars (RLQs) imaged by the WFPC2 on board of HST. The considered objects (z<0.5) are always well resolved and their host galaxies satisfactorily modelled…

天体物理学 · 物理学 2007-05-23 A. Treves , N. Carangelo , R. Falomo , C. M. Urry , M. O'Dowd , R. Scarpa

Using HST observations of 147 host galaxies of low-mass black holes (BHs), we systematically study the structures and scaling relations of these active galaxies. Our sample is selected to have central BHs with virial masses ~10^5-10^6 solar…

宇宙学与河外天体物理 · 物理学 2011-11-09 Yan-Fei Jiang , Jenny E. Greene , Luis C. Ho , Ting Xiao , Aaron J. Barth

(Abridged) We complete the census of nuclear X-ray activity in 100 early type Virgo galaxies observed by the Chandra X-ray Telescope as part of the AMUSE-Virgo survey, down to a (3sigma) limiting luminosity of 3.7E+38 erg/s over 0.5-7 keV.…

高能天体物理现象 · 物理学 2015-05-18 Elena Gallo , Tommaso Treu , Philip J. Marshall , Jong-Hak Woo , Christian Leipski , Robert Antonucci

We present measurements of black hole masses and Eddington ratios for a sample of 38 bright (M$_{1450}$ < -24.4 mag) quasars at 5.8 < z < 7.5, derived from VLT/X-shooter near-IR spectroscopy of their broad CIV and MgII emission lines. The…

We report on the analysis of the photometric and spectroscopic properties of a sample of 29 low redshift (z<0.6) QSOs for which both HST WFPC2 images and ultraviolet HST FOS spectra are available. For each object we measure the R band…

天体物理学 · 物理学 2009-11-11 Marzia Labita , Aldo Treves , Renato Falomo , Michela Uslenghi

Ultra-luminous X-ray sources (ULXs) are off-nuclear X-ray sources in nearby galaxies with X-ray luminosities $\geq$ 10$^{39}$ erg s$^{-1}$. The measurement of the black hole (BH) masses of ULXs is a long-standing problem. Here we estimate…

高能天体物理现象 · 物理学 2015-06-23 Xin-Lin Zhou

We present an analysis of twenty tidal disruption event (TDE) host galaxies observed with the MUSE integral-field spectrograph on ESO VLT. We investigate the presence of extended emission line regions (EELRs) and study stellar populations…

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