SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:kth-84607"
 

Search: onr:"swepub:oai:DiVA.org:kth-84607" > Search for broad ab...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist
  • Iyudin, Anatoli F. (author)

Search for broad absorption lines in spectra of stars in the field of supernova remnant RX J0852.0-4622 (Vela Jr.)

  • Article/chapterEnglish2010

Publisher, publication year, extent ...

  • 2010-09-16
  • EDP Sciences,2010
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:kth-84607
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-84607URI
  • https://doi.org/10.1051/0004-6361/201014031DOI
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51679URI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

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

Notes

  • QC 20120213
  • authorCount :7
  • Aims. Supernova remnant (SNR) RX J0852.0-4622 is one of the youngest and is most likely the closest among known Galactic SNRs. It was detected in X-rays, the (44)Ti gamma-line, and radio. We obtain and analyze medium-resolution spectra of 14 stars in the direction towards the SNR RX J0852.0-4622 in an attempt to detect broad absorption lines of unshocked ejecta against background stars. Methods. Spectral synthesis is performed for all the stars in the wavelength range of 3740-4020 angstrom to extract the broad absorption lines of Ca II related to the SNR RX J0852.0-4622. Results. We do not detect any broad absorption line and place a 3 sigma upper limit on the relative depths of <0.04 for the broad Ca II absorption produced by the SNR. We detect narrow low and high velocity absorption components of Ca II. High velocity vertical bar V(LSR)vertical bar similar to 100-140 km s(-1) components are attributed to radiative shocks in clouds engulfed by the old Vela SNR. The upper limit to the absorption line strength combined with the width and flux of the (44)Ti gamma-ray line 1.16 MeV lead us to conclude that SNR RX J0852.0-4622 was probably produced by an energetic SN Ic explosion.

Subject headings and genre

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

  • Pakhomov, Y. V. (author)
  • Chugai, N. N. (author)
  • Greiner, J. (author)
  • Axelsson, MagnusStockholms universitet,Institutionen för astronomi(Swepub:su)aaxe (author)
  • Larsson, StefanStockholms universitet,Institutionen för astronomi(Swepub:su)slars (author)
  • Ryabchikova, T. A. (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Astronomy and Astrophysics: EDP Sciences519:9, s. A86-0004-63611432-0746

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