onr:"swepub:oai:DiVA.org:su-198635"
Search: onr:"swepub:oai:DiVA.org:su-198635" > Probing the progeni...
- 1 of 1
- Previous record
- Next record
- To hitlist
- Clark, Peter (author)
Probing the progenitors of Type Ia supernovae using circumstellar material interaction signatures
- Article/chapterEnglish2021
Publisher, publication year, extent ...
- 2021-07-16
- Oxford University Press (OUP),2021
- printrdacarrier
Numbers
- LIBRIS-ID:oai:DiVA.org:su-198635
- https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-198635URI
- https://doi.org/10.1093/mnras/stab2038DOI
Supplementary language notes
- Language:English
- Summary in:English
Part of subdatabase
- SwePubSwePub
Classification
Notes
- This work aims to study different probes of Type Ia supernova (SN Ia) progenitors that have been suggested to be linked to the presence of circumstellar material (CSM). In particular, we have investigated, for the first time, the link between narrow blueshifted Na I D absorption profiles and the presence and strength of the broad high-velocity Ca II near-infrared triplet absorption features seen in SNe la around maximum light. With the probes exploring different distances from the SN; Na I D > 10(17) cm, high-velocity Ca TT features < 10(15) cm. For this, we have used a new intermediate-resolution X-shooter spectral sample of 15 SNe Ia. We do not identify a link between these two probes, implying either that, one (or both) is not physically related to the presence of CSM or that the occurrence of CSM at the distance explored by one probe is not linked to its presence at the distance probed by the other. However, the previously identified statistical excess in the presence of blueshifted (over redshifted) Na I D absorption is confirmed in this sample at high significance and is found to be stronger in SNe Ia hosted by late-type galaxies. This excess is difficult to explain as being from an interstellar-medium origin as has been suggested by some recent modelling, as such an origin is not expected to show a bias for blueshifted absorption. However, a circumstellar origin for these features also appears unsatisfactory based on our new results, given the lack of link between the two probes of CSM investigated.
Subject headings and genre
- NATURVETENSKAP Fysik Astronomi, astrofysik och kosmologi hsv//swe
- NATURAL SCIENCES Physical Sciences Astronomy, Astrophysics and Cosmology hsv//eng
- circumstellar matter
- supernovae: general
- distance scale
Added entries (persons, corporate bodies, meetings, titles ...)
- Maguire, Kate (author)
- Bulla, MattiaStockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC)(Swepub:su)mbull (author)
- Galbany, Lluís (author)
- Sullivan, Mark (author)
- Anderson, Joseph P. (author)
- Smartt, Stephen J. (author)
- Stockholms universitetInstitutionen för astronomi (creator_code:org_t)
Related titles
- In:Monthly notices of the Royal Astronomical Society: Oxford University Press (OUP)507:3, s. 4367-43880035-87111365-2966
Internet link
Find in a library
- Monthly notices of the Royal Astronomical Society (Search for host publication in LIBRIS)
To the university's database
- 1 of 1
- Previous record
- Next record
- To hitlist
Find more in SwePub
- By the author/editor
- Clark, Peter
- Maguire, Kate
- Bulla, Mattia
- Galbany, Lluís
- Sullivan, Mark
- Anderson, Joseph ...
- show more...
- Smartt, Stephen ...
- show less...
- About the subject
-
- NATURAL SCIENCES
- NATURAL SCIENCES
- and Physical Science ...
- and Astronomy Astrop ...
- Articles in the publication
- Monthly notices ...
- By the university
- Stockholm University
Search outside SwePub
- Extend your search to:
- Google Book Search
- Google Scholar
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.
- Copyright © LIBRIS - National Library Systems
- LIBRIS.kb.se
