SwePub
Sök i LIBRIS databas

  Extended search

WFRF:(Misra A)
 

Search: WFRF:(Misra A) > (2015-2019) > SN 2015ba :

SN 2015ba : a Type IIP supernova with a long plateau

Dastidar, Raya (author)
Misra, Kuntal (author)
Hosseinzadeh, G. (author)
show more...
Pastorello, A. (author)
Pumo, M. L. (author)
Valenti, S. (author)
McCully, C. (author)
Tomasella, L. (author)
Arcavi, I (author)
Elias-Rosa, N. (author)
Singh, Mridweeka (author)
Gangopadhyay, Anjasha (author)
Howell, D. A. (author)
Morales-Garoffolo, Antonia (author)
Zampieri, L. (author)
Kumar, Brijesh (author)
Turatto, M. (author)
Benetti, S. (author)
Tartaglia, Leonardo (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Ochner, P. (author)
Sahu, D. K. (author)
Anupama, G. C. (author)
Pandey, S. B. (author)
show less...
 (creator_code:org_t)
2018-06-21
2018
English.
In: Monthly notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 479:2, s. 2421-2442
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We present optical photometry and spectroscopy from about a week after explosion to similar to 272 d of an atypical Type IIP supernova, SN 2015ba, which exploded in the edge-on galaxy IC 1029. SN 2015ba is a luminous event with an absolute V-band magnitude of -17.1 +/- 0.2 mag at 50 d since explosion and has a long plateau lasting for similar to 123 d. The distance to the SN is estimated to be 34.8 +/- 0.7 Mpc using the expanding photosphere and standard candle methods. High-velocity H Balmer components constant with time are observed in the late-plateau phase spectra of SN 2015ba, which suggests a possible role of circumstellar interaction at these phases. Both hydrodynamical and analytical modelling suggest a massive progenitor of SN 2015ba with a pre-explosion mass of 24-26 M-circle dot. However, the nebular spectra of SN 2015ba exhibit insignificant levels of oxygen, which is otherwise expected from a massive progenitor. This might be suggestive of the non-monotonical link between O-core masses and the zero-age main sequence mass of pre-supernova stars and/or uncertainties in the mixing scenario in the ejecta of supernovae.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

techniques: photometric
techniques: spectroscopic
supernovae: general
supernovae: individual: SN 2015ba
galaxies: individual: IC 1029

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

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