SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-187650"
 

Search: onr:"swepub:oai:DiVA.org:su-187650" > Helium-rich Superlu...

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

Helium-rich Superluminous Supernovae from the Zwicky Transient Facility

Yan, Lin (author)
Perley, D. A. (author)
Schulze, S. (author)
show more...
Lunnan, Ragnhild (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Sollerman, Jesper (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
De, K. (author)
Chen, Z. H. (author)
Fremling, C. (author)
Gal-Yam, A. (author)
Taggart, K. (author)
Chen, Ting-Wan (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Andreoni, I. (author)
Bellm, E. C. (author)
Cunningham, V. (author)
Dekany, R. (author)
Duev, D. A. (author)
Fransson, Claes (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Laher, R. R. (author)
Hankins, M. (author)
Ho, A. Y. Q. (author)
Jencson, J. E. (author)
Kaye, S. (author)
Kulkarni, S. R. (author)
Kasliwal, M. M. (author)
Golkhou, V. Z. (author)
Graham, M. (author)
Masci, F. J. (author)
Miller, A. A. (author)
Neill, J. D. (author)
Ofek, E. (author)
Porter, M. (author)
Mroz, P. (author)
Reiley, D. (author)
Riddle, R. (author)
Rigault, M. (author)
Rusholme, B. (author)
Shupe, D. L. (author)
Soumagnac, M. T. (author)
Smith, R. (author)
Tartaglia, Leonardo (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Yao, Y. (author)
Yaron, O. (author)
show less...
 (creator_code:org_t)
2020-10-07
2020
English.
In: Astrophysical Journal Letters. - : American Astronomical Society. - 2041-8205 .- 2041-8213. ; 902:1
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Helium is expected to be present in the massive ejecta of some hydrogen-poor superluminous supernovae (SLSN-I). However, until now only one event has been identified with He features in its photospheric spectra (PTF10hgi). We present the discovery of a new He-rich SLSN-I, ZTF19aawfbtg (SN2019hge), atz = 0.0866. This event has more than 10 optical spectra at phases from -41 to +103 days relative to the peak, most of which match well with that of PTF10hgi. Confirmation comes from a near-IR spectrum taken at +34 days, revealing Heifeatures with P-Cygni profiles at 1.083 and 2.058 mu m. Using the optical spectra of PTF10hgi and SN2019hge as templates, we examined 70 other SLSNe-I discovered by Zwicky Transient Facility in the first two years of operation and found five additional SLSNe-I with distinct He-features. The excitation of Heiatoms in normal core-collapse supernovae requires nonthermal radiation, as proposed by previous studies. These He-rich events cannot be explained by the traditional(56)Ni mixing model because of their blue spectra, high peak luminosities, and long rise timescales. Magnetar models offer a possible solution since pulsar winds naturally generate high-energy particles, potential sources of nonthermal excitation. An alternative model is the interaction between the ejecta and dense H-poor circumstellar material, which may be supported by observed undulations in the light curves. These six SLSNe-Ib have relatively low-peak luminosities (rest frameM(g) = -20.06 0.16).

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

Supernovae
Type Ib supernovae

Publication and Content Type

ref (subject category)
art (subject category)

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