SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:su-231539"
 

Search: onr:"swepub:oai:DiVA.org:su-231539" > The carbon-rich typ...

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

The carbon-rich type Ic supernova 2016adj in the iconic dust lane of Centaurus A : Potential signatures of an interaction with circumstellar hydrogen

Stritzinger, M. D. (author)
Baron, E. (author)
Taddia, F. (author)
show more...
Burns, C. R. (author)
Fraser, M. (author)
Galbany, L. (author)
Holmbo, S. (author)
Hoeflich, P. (author)
Morrell, N. (author)
Arndt, L. S. (author)
Hsiao, E. Y. (author)
Pearson Johansson, Joel, 1984- (author)
Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)
Karamehmetoglu, E. (author)
Kuncarayakti, H. (author)
Lyman, J. (author)
Moriya, T. J. (author)
Phan, K. (author)
Phillips, M. M. (author)
Anderson, J. P. (author)
Ashall, C. (author)
Brown, P. J. (author)
Castellón, S. (author)
Della Valle, M. (author)
González-Gaitán, S. (author)
Gromadzki, M. (author)
Handberg, R. (author)
Lu, J. (author)
Nicholl, M. (author)
Shahbandeh, M. (author)
show less...
 (creator_code:org_t)
2024
2024
English.
In: Astronomy and Astrophysics. - 0004-6361 .- 1432-0746. ; 686
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We present a comprehensive data set of supernova (SN) 2016adj located within the central dust lane of Centaurus A. SN 2016adj is significantly reddened and after correcting the peak apparent B-band magnitude (mB = 17.48 ± 0.05) for Milky Way reddening and our inferred host-galaxy reddening parameters (i.e., RVhost = 5.7±0.7 and AVhost = 6.3 ± 0.2 mag), we estimated it reached a peak absolute magnitude of MB ∼ −18. A detailed inspection of the optical and near-infrared (NIR) spectroscopic time series reveals a carbon-rich SN Ic and not a SN Ib/IIb as previously suggested in the literature. The NIR spectra show prevalent carbon-monoxide formation occurring already by +41 days past B-band maximum, which is ≈11 days earlier than previously reported in the literature for this object. Interestingly, around two months past maximum, the NIR spectrum of SN 2016adj begins to exhibit H features, with a +97 days medium resolution spectrum revealing both Paschen and Bracket lines with absorption minima of ∼2000 km s−1, full-width-half-maximum emission velocities of ∼1000 km s−1, and emission line ratios consistent with a dense emission region. We speculate that these attributes are due to a circumstellar interaction (CSI) between the rapidly expanding SN ejecta and a H-rich shell of material that formed during the pre-SN phase. A bolometric light curve was constructed and a semi-analytical model fit suggests the SN synthesized 0.5 M⊙ of 56Ni and ejected 4.7 M⊙ of material, though these values should be approached with caution given the large uncertainties associated with the adopted reddening parameters and known light echo emission. Finally, inspection of the Hubble Space Telescope archival data yielded no progenitor detection.

Subject headings

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

Keyword

supernovae: general
supernovae: individual: 2016adj

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