Scary Barbie: An Extremely Energetic, Long-duration Tidal Disruption Event Candidate without a Detected Host Galaxy at z=0.995

被引:10
作者
Subrayan, Bhagya M. [1 ]
Milisavljevic, Dan [1 ,2 ]
Chornock, Ryan [3 ]
Margutti, Raffaella [3 ]
Alexander, Kate D. [4 ,5 ]
Ramakrishnan, Vandana [1 ]
Duffell, Paul C. [1 ]
Dickinson, Danielle A. [1 ]
Lee, Kyoung-Soo [1 ]
Giannios, Dimitrios [1 ]
Lentner, Geoffery [1 ]
Linvill, Mark [1 ]
Garretson, Braden [1 ]
Graham, Matthew J. [6 ]
Stern, Daniel [7 ]
Brethauer, Daniel [3 ]
Duong, Tien [3 ]
Jacobson-Galan, Wynn [3 ]
LeBaron, Natalie [3 ]
Matthews, David [3 ]
Sears, Huei [8 ,9 ]
Venkatraman, Padma [3 ]
机构
[1] Purdue Univ, Dept Phys & Astron, 525 Northwestern Ave, W Lafayette, IN 47907 USA
[2] Purdue Univ, Integrat Data Sci Initiat, W Lafayette, IN 47907 USA
[3] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[4] Univ Arizona, Dept Astron, 933 North Cherry Ave, Tucson, AZ 85721 USA
[5] Univ Arizona, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA
[6] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA
[7] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[8] Northwestern Univ, Ctr Interdisciplinary Explorat & Res Astrophys CIE, Evanston, IL 60202 USA
[9] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA
基金
加拿大创新基金会; 美国国家科学基金会; 美国国家航空航天局;
关键词
ACTIVE GALACTIC NUCLEI; STELLAR POPULATION SYNTHESIS; BLACK-HOLE MASSES; RAPID TURN-ON; LIGHT CURVES; RELATIVISTIC JETS; STAR-FORMATION; EMISSION-LINE; SCALING RELATIONS; ACCRETION DISKS;
D O I
10.3847/2041-8213/accf1a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report multiwavelength observations and characterization of the ultraluminous transient AT 2021lwx (ZTF20abrbeie; aka "Barbie") identified in the alert stream of the Zwicky Transient Facility (ZTF) using a Recommender Engine For Intelligent Transient Tracking filter on the ANTARES alert broker. From a spectroscopically measured redshift of 0.995, we estimate a peak-observed pseudo-bolometric luminosity of log (L-max/[erg s(-1)]) = 45.7 from slowly fading ztf-g and ztf-r light curves spanning over 1000 observer-frame days. The host galaxy is not detected in archival Pan-STARRS observations (g > 23.3 mag), implying a lower limit to the outburst amplitude of more than 5 mag relative to the quiescent host galaxy. Optical spectra exhibit strong emission lines with narrow cores from the H Balmer series and ultraviolet semi-forbidden lines of Si III] lambda 1892,. C III] lambda 1909, and.C II] lambda 2325. Typical nebular lines in Active Galactic Nucleus (AGN).spectra from ions such as [O II] and [O III] are not detected. These spectral features, along with the smooth light curve that is unlike most AGN flaring activity and the luminosity that exceeds any observed or theorized supernova, lead us to conclude that AT 2021lwx is most likely an extreme tidal disruption event (TDE). Modeling of ZTF photometry with MOSFiT suggests that the TDE was between a approximate to 14M(circle dot) star and a supermassive black hole of mass M-BH similar to 10(8)M(circle dot). Continued monitoring of the still-evolving light curve along with deep imaging of the field once AT 2021lwx has faded can test this hypothesis and potentially detect the host galaxy.
引用
收藏
页数:11
相关论文
共 128 条
  • [1] Radio Properties of Tidal Disruption Events
    Alexander, Kate D.
    van Velzen, Sjoert
    Horesh, Assaf
    Zauderer, B. Ashley
    [J]. SPACE SCIENCE REVIEWS, 2020, 216 (05)
  • [2] A very luminous jet from the disruption of a star by a massive black hole
    Andreoni, Igor
    Coughlin, Michael W.
    Perley, Daniel A.
    Yao, Yuhan
    Lu, Wenbin
    Cenko, S. Bradley
    Kumar, Harsh
    Anand, Shreya
    Ho, Anna Y. Q.
    Kasliwal, Mansi M.
    Postigo, Antonio de Ugarte
    Sagues-Carracedo, Ana
    Schulze, Steve
    Kann, D. Alexander
    Kulkarni, S. R.
    Sollerman, Jesper
    Tanvir, Nial
    Rest, Armin
    Izzo, Luca
    Somalwar, Jean J.
    Kaplan, David L.
    Ahumada, Tomas
    Anupama, G. C.
    Auchettl, Katie
    Barway, Sudhanshu
    Bellm, Eric C.
    Bhalerao, Varun
    Bloom, Joshua S.
    Bremer, Michael
    Bulla, Mattia
    Burns, Eric
    Campana, Sergio
    Chandra, Poonam
    Charalampopoulos, Panos
    Cooke, Jeff
    D'Elia, Valerio
    Das, Kaustav Kashyap
    Dobie, Dougal
    Fernandez, Jose Feliciano Agui
    Freeburn, James
    Fremling, Cristoffer
    Gezari, Suvi
    Goode, Simon
    Graham, Matthew J.
    Hammerstein, Erica
    Karambelkar, Viraj R.
    Kilpatrick, Charles D.
    Kool, Erik C.
    Krips, Melanie
    Laher, Russ R.
    [J]. NATURE, 2022, 612 (7940) : 430 - +
  • [3] Angione R. J., 1972, P IAU S, V44, P171
  • [4] [Anonymous], 2022, Zwicky Transient Facility Image Service, DOI DOI 10.26131/IRSA539
  • [5] The largest blueshifts of the [O III] emission line in two narrow-line quasars
    Aoki, K
    Kawaguchi, T
    Ohta, K
    [J]. ASTROPHYSICAL JOURNAL, 2005, 618 (02) : 601 - 608
  • [6] A CONTINUUM OF H- TO He-RICH TIDAL DISRUPTION CANDIDATES WITH A PREFERENCE FOR E plus A GALAXIES
    Arcavi, Iair
    Gal-Yam, Avishay
    Sullivan, Mark
    Pan, Yen-Chen
    Cenko, S. Bradley
    Horesh, Assaf
    Ofek, Eran O.
    De Cia, Annalisa
    Yan, Lin
    Yang, Chen-Wei
    Howell, D. A.
    Tal, David
    Kulkarni, Shrinivas R.
    Tendulkar, Shriharsh P.
    Tang, Sumin
    Xu, Dong
    Sternberg, Assaf
    Cohen, Judith G.
    Bloom, Joshua S.
    Nugent, Peter E.
    Kasliwal, Mansi M.
    Perley, Daniel A.
    Quimby, Robert M.
    Miller, Adam A.
    Theissen, Christopher A.
    Laher, Russ R.
    [J]. ASTROPHYSICAL JOURNAL, 2014, 793 (01)
  • [7] The metallicities of the broad emission line regions in the nitrogen-loudest quasars
    Batra, Neelam Dhanda
    Baldwin, Jack A.
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2014, 439 (01) : 771 - 787
  • [8] QUASAR OPTICAL VARIABILITY IN THE PALOMAR-QUEST SURVEY
    Bauer, Anne
    Baltay, Charles
    Coppi, Paolo
    Ellman, Nancy
    Jerke, Jonathan
    Rabinowitz, David
    Scalzo, Richard
    [J]. ASTROPHYSICAL JOURNAL, 2009, 696 (02) : 1241 - 1256
  • [9] The Zwicky Transient Facility: System Overview, Performance, and First Results
    Bellm, Eric C.
    Kulkarni, Shrinivas R.
    Graham, Matthew J.
    Dekany, Richard
    Smith, Roger M.
    Riddle, Reed
    Masci, Frank J.
    Helou, George
    Prince, Thomas A.
    Adams, Scott M.
    Barbarino, C.
    Barlow, Tom
    Bauer, James
    Beck, Ron
    Belicki, Justin
    Biswas, Rahul
    Blagorodnova, Nadejda
    Bodewits, Dennis
    Bolin, Bryce
    Brinnel, Valery
    Brooke, Tim
    Bue, Brian
    Bulla, Mattia
    Burruss, Rick
    Cenko, S. Bradley
    Chang, Chan-Kao
    Connolly, Andrew
    Coughlin, Michael
    Cromer, John
    Cunningham, Virginia
    De, Kishalay
    Delacroix, Alex
    Desai, Vandana
    Duev, Dmitry A.
    Eadie, Gwendolyn
    Farnham, Tony L.
    Feeney, Michael
    Feindt, Ulrich
    Flynn, David
    Franckowiak, Anna
    Frederick, S.
    Fremling, C.
    Gal-Yam, Avishay
    Gezari, Suvi
    Giomi, Matteo
    Goldstein, Daniel A.
    Golkhou, V. Zach
    Goobar, Ariel
    Groom, Steven
    Hacopians, Eugean
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2019, 131 (995)
  • [10] Black Hole Galaxy Scaling Relationships for Active Galactic Nuclei with Reverberation Masses
    Bentz, Misty C.
    Manne-Nicholas, Emily
    [J]. ASTROPHYSICAL JOURNAL, 2018, 864 (02)