PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk
Abstract
We present the discovery of PS18kh, a tidal disruption event discovered at the center of SDSS J075654.53+341543.6 (d ≃ 322 Mpc) by the Pan-STARRS Survey for Transients. Our data set includes pre-discovery survey data from Pan-STARRS, the All-sky Automated Survey for Supernovae, and the Asteroid Terrestrial-impact Last Alert System as well as high-cadence, multiwavelength follow-up data from ground-based telescopes and Swift, spanning from 56 days before peak light until 75 days after. The optical/UV emission from PS18kh is well-fit as a blackbody with temperatures ranging from T ≃ 12,000 K to T ≃ 25,000 K and it peaked at a luminosity of L ≃ 8.8 × 1043 erg s-1. PS18kh radiated E = (3.45 ± 0.22) × 1050 erg over the period of observation, with (1.42 ± 0.20) × 1050 erg being released during the rise to peak. Spectra of PS18kh show a changing, boxy/double-peaked Hα emission feature, which becomes more prominent over time. We use models of non-axisymmetric accretion disks to describe the profile of the Hα line and its evolution. We find that at early times the high accretion rate leads the disk to emit a wind which modifies the shape of the line profile and makes itmore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Org.:
- Pan-STARRS; ASAS-SN; ATLAS Collaboration
- OSTI Identifier:
- 1561939
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 880; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Holoien, T. W. -S., Huber, M. E., Shappee, B. J., Eracleous, M., Auchettl, K., Brown, J. S., Tucker, M. A., Chambers, K. C., Kochanek, C. S., Stanek, K. Z., Rest, A., Bersier, D., Post, R. S., Aldering, G., Ponder, K. A., Simon, J. D., Kankare, E., Dong, D., Hallinan, G., Reddy, N. A., Sanders, R. L., Topping, M. W., Bulger, J., Lowe, T. B., Magnier, E. A., Schultz, A. S. B., Waters, C. Z., Willman, M., Wright, D., Young, D. R., Dong, Subo, Prieto, J. L., Thompson, Todd A., Denneau, L., Flewelling, H., Heinze, A. N., Smartt, S. J., Smith, K. W., Stalder, B., Tonry, J. L., and Weiland, H. PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk. United States: N. p., 2019.
Web. doi:10.3847/1538-4357/ab2ae1.
Holoien, T. W. -S., Huber, M. E., Shappee, B. J., Eracleous, M., Auchettl, K., Brown, J. S., Tucker, M. A., Chambers, K. C., Kochanek, C. S., Stanek, K. Z., Rest, A., Bersier, D., Post, R. S., Aldering, G., Ponder, K. A., Simon, J. D., Kankare, E., Dong, D., Hallinan, G., Reddy, N. A., Sanders, R. L., Topping, M. W., Bulger, J., Lowe, T. B., Magnier, E. A., Schultz, A. S. B., Waters, C. Z., Willman, M., Wright, D., Young, D. R., Dong, Subo, Prieto, J. L., Thompson, Todd A., Denneau, L., Flewelling, H., Heinze, A. N., Smartt, S. J., Smith, K. W., Stalder, B., Tonry, J. L., & Weiland, H. PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk. United States. https://doi.org/10.3847/1538-4357/ab2ae1
Holoien, T. W. -S., Huber, M. E., Shappee, B. J., Eracleous, M., Auchettl, K., Brown, J. S., Tucker, M. A., Chambers, K. C., Kochanek, C. S., Stanek, K. Z., Rest, A., Bersier, D., Post, R. S., Aldering, G., Ponder, K. A., Simon, J. D., Kankare, E., Dong, D., Hallinan, G., Reddy, N. A., Sanders, R. L., Topping, M. W., Bulger, J., Lowe, T. B., Magnier, E. A., Schultz, A. S. B., Waters, C. Z., Willman, M., Wright, D., Young, D. R., Dong, Subo, Prieto, J. L., Thompson, Todd A., Denneau, L., Flewelling, H., Heinze, A. N., Smartt, S. J., Smith, K. W., Stalder, B., Tonry, J. L., and Weiland, H. Thu .
"PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk". United States. https://doi.org/10.3847/1538-4357/ab2ae1. https://www.osti.gov/servlets/purl/1561939.
@article{osti_1561939,
title = {PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk},
author = {Holoien, T. W. -S. and Huber, M. E. and Shappee, B. J. and Eracleous, M. and Auchettl, K. and Brown, J. S. and Tucker, M. A. and Chambers, K. C. and Kochanek, C. S. and Stanek, K. Z. and Rest, A. and Bersier, D. and Post, R. S. and Aldering, G. and Ponder, K. A. and Simon, J. D. and Kankare, E. and Dong, D. and Hallinan, G. and Reddy, N. A. and Sanders, R. L. and Topping, M. W. and Bulger, J. and Lowe, T. B. and Magnier, E. A. and Schultz, A. S. B. and Waters, C. Z. and Willman, M. and Wright, D. and Young, D. R. and Dong, Subo and Prieto, J. L. and Thompson, Todd A. and Denneau, L. and Flewelling, H. and Heinze, A. N. and Smartt, S. J. and Smith, K. W. and Stalder, B. and Tonry, J. L. and Weiland, H.},
abstractNote = {We present the discovery of PS18kh, a tidal disruption event discovered at the center of SDSS J075654.53+341543.6 (d ≃ 322 Mpc) by the Pan-STARRS Survey for Transients. Our data set includes pre-discovery survey data from Pan-STARRS, the All-sky Automated Survey for Supernovae, and the Asteroid Terrestrial-impact Last Alert System as well as high-cadence, multiwavelength follow-up data from ground-based telescopes and Swift, spanning from 56 days before peak light until 75 days after. The optical/UV emission from PS18kh is well-fit as a blackbody with temperatures ranging from T ≃ 12,000 K to T ≃ 25,000 K and it peaked at a luminosity of L ≃ 8.8 × 1043 erg s-1. PS18kh radiated E = (3.45 ± 0.22) × 1050 erg over the period of observation, with (1.42 ± 0.20) × 1050 erg being released during the rise to peak. Spectra of PS18kh show a changing, boxy/double-peaked Hα emission feature, which becomes more prominent over time. We use models of non-axisymmetric accretion disks to describe the profile of the Hα line and its evolution. We find that at early times the high accretion rate leads the disk to emit a wind which modifies the shape of the line profile and makes it bell-shaped. At late times, the wind becomes optically thin, allowing the non-axisymmetric perturbations to show up in the line profile. The line-emitting portion of the disk extends from r in ~ 60r g to an outer radius of r out ~ 1400r g and the perturbations can be represented either as an eccentricity in the outer rings of the disk or as a spiral arm in the inner disk.},
doi = {10.3847/1538-4357/ab2ae1},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 880,
place = {United States},
year = {Thu Aug 01 00:00:00 EDT 2019},
month = {Thu Aug 01 00:00:00 EDT 2019}
}
Web of Science
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Works referencing / citing this record:
Evidence for rapid disc formation and reprocessing in the X-ray bright tidal disruption event candidate AT 2018fyk
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Self-intersection of the fallback stream in tidal disruption events
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Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS
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The Spectral Evolution of AT 2018dyb and the Presence of Metal Lines in Tidal Disruption Events
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The ASAS-SN catalogue of variable stars – V. Variables in the Southern hemisphere
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An Unusual Mid-infrared Flare in a Type 2 AGN: An Obscured Turning-on AGN or Tidal Disruption Event?
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Evidence for rapid disk formation and reprocessing in the X-ray bright tidal disruption event AT 2018fyk
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The ASAS-SN Catalog of Variable Stars V: Variables in the Southern Hemisphere
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