SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-104569"
 

Search: onr:"swepub:oai:DiVA.org:su-104569" > Low luminosity Type...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist
  • Spiro, S. (author)

Low luminosity Type II supernovae - II. Pointing towards moderate mass precursors

  • Article/chapterEnglish2014

Publisher, publication year, extent ...

  • 2014-02-21
  • Oxford University Press (OUP),2014
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-104569
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-104569URI
  • https://doi.org/10.1093/mnras/stu156DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

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

Notes

  • AuthorCount:41;
  • We present new data for five underluminous Type II-plateau supernovae (SNe IIP), namely SN 1999gn, SN 2002gd, SN 2003Z, SN 2004eg and SN 2006ov. This new sample of low-luminosity SNe IIP (LL SNe IIP) is analysed together with similar objects studied in the past. All of them show a flat light-curve plateau lasting about 100 d, an underluminous late-time exponential tail, intrinsic colours that are unusually red, and spectra showing prominent and narrow P Cygni lines. A velocity of the ejected material below 10(3) km s(-1) is inferred from measurements at the end of the plateau. The Ni-56 masses ejected in the explosion are very small (< 10(-2) M-circle dot). We investigate the correlations among Ni-56 mass, expansion velocity of the ejecta and absolute magnitude in the middle of the plateau, confirming the main findings of Hamuy, according to which events showing brighter plateau and larger expansion velocities are expected to produce more Ni-56. We propose that these faint objects represent the LL tail of a continuous distribution in parameters space of SNe IIP. The physical properties of the progenitors at the explosion are estimated through the hydrodynamical modelling of the observables for two representative events of this class, namely SN 2005cs and SN 2008in. We find that the majority of LL SNe IIP, and quite possibly all, originate in the core collapse of intermediate-mass stars, in the mass range 10-15 M-circle dot.

Subject headings and genre

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

  • Pastorello, A. (author)
  • Pumo, M. L. (author)
  • Zampieri, L. (author)
  • Turatto, M. (author)
  • Smartt, S. J. (author)
  • Benetti, S. (author)
  • Cappellaro, E. (author)
  • Valenti, S. (author)
  • Agnoletto, I. (author)
  • Altavilla, G. (author)
  • Aoki, T. (author)
  • Brocato, E. (author)
  • Corsini, E. M. (author)
  • Di Cianno, A. (author)
  • Elias-Rosa, N. (author)
  • Hamuy, M. (author)
  • Enya, K. (author)
  • Fiaschi, M. (author)
  • Folatelli, G. (author)
  • Desidera, S. (author)
  • Harutyunyan, A. (author)
  • Howell, D. A. (author)
  • Kawka, A. (author)
  • Kobayashi, Y. (author)
  • Leibundgut, B. (author)
  • Minezaki, T. (author)
  • Navasardyan, H. (author)
  • Nomoto, K. (author)
  • Mattila, S. (author)
  • Pietrinferni, A. (author)
  • Pignata, G. (author)
  • Raimondo, G. (author)
  • Salvo, M. (author)
  • Schmidt, B. P. (author)
  • Sollerman, JesperStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)solle (author)
  • Spyromilio, J. (author)
  • Taubenberger, S. (author)
  • Valentini, G. (author)
  • Vennes, S. (author)
  • Yoshii, Y. (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Monthly notices of the Royal Astronomical Society: Oxford University Press (OUP)439:3, s. 2873-28920035-87111365-2966

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