Article

Integral Field Spectroscopy of 13 Tidal Disruption Event Hosts from the Zwicky Transient Facility Survey

Erica HammersteinAstrophysics Science Division, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USAS. B. CenkoAstrophysics Science Division, NASA Goddard Space Flight Center, 8800 Greenbelt Road, Greenbelt, MD 20771, USASuvi GezariDepartment of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles Street, Baltimore, MD 21218, USASylvain VeilleuxDepartment of Astronomy, University of Maryland, College Park, MD 20742, USA; [email protected]Brendan O’ConnorAstronomy, Physics and Statistics Institute of Sciences (APSIS), The George Washington University, Washington, DC 20052, USASjoert van VelzenLeiden Observatory, Leiden University, Postbus 9513, 2300 RA Leiden, The NetherlandsCharlotte WardDepartment of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USAYuhan YaoCahill Center for Astrophysics, California Institute of Technology, MC 249-17, 1200 E. California Boulevard, Pasadena, CA, 91125, USAM. J. GrahamDepartment of Astronomy, California Institute of Technology, 1200 E. California Boulevard, Pasadena, CA, 91125, USA

2023en

ABI

Abstract

Abstract 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 galaxy characteristics among TDE host populations suggests that they may serve to boost the TDE rate in such galaxies by influencing the nuclear stellar dynamics. We present the first population study of integral field spectroscopy for 13 TDE host galaxies across all spectral classes and X-ray brightnesses with the purpose of investigating their large-scale properties. We derive the black hole masses via stellar kinematics (i.e., the M – σ relation) and find masses in the range <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mn>5.0</mml:mn> <mml:mo>≲</mml:mo> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>BH</mml:mi> </mml:mrow> </mml:msub> <mml:mrow> <mml:mo stretchy="true">/</mml:mo> </mml:mrow> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>≲</mml:mo> <mml:mn>8.0</mml:mn> </mml:math> , with a distribution dominated by black holes with M BH ∼ 10 6 M ⊙ . We find one object with M BH ≳ 10 8 M ⊙ , above the “Hills mass”, which if the disrupted star was of solar type, allows a lower limit of a ≳ 0.16 to be placed on its spin, lending further support to the proposed connection between featureless TDEs and jetted TDEs. We also explore the level of rotational support in the TDE hosts, quantified by ( V / σ ) e , a parameter that has been shown to correlate with the stellar age and may explain the peculiar host-galaxy preferences of TDEs. We find that the TDE hosts exhibit a broad range in ( V / σ ) e following a similar distribution as E + A galaxies, which have been shown to be overrepresented among TDE host populations.

Identifiers

DOI: 10.3847/1538-4357/acfb84

Citations and references

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