SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-188182"
 

Search: onr:"swepub:oai:DiVA.org:su-188182" > The tidal disruptio...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist
  • Short, P. (author)

The tidal disruption event AT2018hyz-I. Double-peaked emission lines and a flat Balmer decrement

  • Article/chapterEnglish2020

Publisher, publication year, extent ...

  • 2020-09-02
  • Oxford University Press (OUP),2020
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-188182
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-188182URI
  • https://doi.org/10.1093/mnras/staa2065DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • We present results from spectroscopic observations of AT 2018hyz, a transient discovered by the All-Sky Automated Survey for Supernova survey at an absolute magnitude of M-V similar to -20.2 mag, in the nucleus of a quiescent galaxy with strong Balmer absorption lines. AT 2018hyz shows a blue spectral continuum and broad emission lines, consistent with previous TDE candidates. High cadence follow-up spectra show broad Balmer lines and He I in early spectra, with He II making an appearance after similar to 70-100 d. The Balmer lines evolve from a smooth broad profile, through a boxy, asymmetric double-peaked phase consistent with accretion disc emission, and back to smooth at late times. The Balmer lines are unlike typical active galactic nucleus in that they show a flat Balmer decrement (H alpha/H beta similar to 1.5), suggesting the lines are collisionally excited rather than being produced via photoionization. The flat Balmer decrement together with the complex profiles suggests that the emission lines originate in a disc chromosphere, analogous to those seen in cataclysmic variables. The low optical depth of material due to a possible partial disruption may be what allows us to observe these double-peaked, collisionally excited lines. The late appearance of He II may be due to an expanding photosphere or outflow, or late-time shocks in debris collisions.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Nicholl, M. (author)
  • Lawrence, A. (author)
  • Gomez, S. (author)
  • Arcavi, I. (author)
  • Wevers, T. (author)
  • Leloudas, G. (author)
  • Schulze, S. (author)
  • Anderson, J. P. (author)
  • Berger, E. (author)
  • Blanchard, P. K. (author)
  • Burke, J. (author)
  • Castro Segura, N. (author)
  • Charalampopoulos, P. (author)
  • Chornock, R. (author)
  • Galbany, L. (author)
  • Gromadzki, M. (author)
  • Herzog, L. J. (author)
  • Hiramatsu, D. (author)
  • Horne, Keith (author)
  • Hosseinzadeh, G. (author)
  • Howell, D. Andrew (author)
  • Ihanec, N. (author)
  • Inserra, C. (author)
  • Kankare, E. (author)
  • Maguire, K. (author)
  • McCully, C. (author)
  • Müller Bravo, T. E. (author)
  • Onori, F. (author)
  • Sollerman, JesperStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)solle (author)
  • Young, D. R. (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Monthly notices of the Royal Astronomical Society: Oxford University Press (OUP)498:3, s. 4119-41330035-87111365-2966

Internet link

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view