- Abstract:
-
A spectroscopic analysis has been undertaken for the B-type multiple systems (excluding those with supergiant primaries) in the VLT-FLAMES Tarantula Survey (VFTS). Projected rotational velocities, ve sin i, for the primaries have been estimated using a Fourier Transform technique and confirmed by fitting rotationally broadened profiles. A subset of 33 systems with ve sin i80 km s1 have been analysed using a TLUSTY grid of model atmospheres to estimate stellar parameters and surface abundances...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 394.4kb)
-
- Publisher copy:
- 10.1051/0004-6361/201629982
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
- Publisher:
- EDP Sciences Publisher's website
- Journal:
- Astronomy and Astrophysics Journal website
- Volume:
- 603
- Pages:
- Article: A91
- Publication date:
- 2017-07-12
- Acceptance date:
- 2017-04-10
- DOI:
- EISSN:
-
1432-0746
- ISSN:
-
0004-6361
- Pubs id:
-
pubs:709744
- URN:
-
uri:e4a9ff88-65ad-4836-9193-40afbbeb7924
- UUID:
-
uuid:e4a9ff88-65ad-4836-9193-40afbbeb7924
- Local pid:
- pubs:709744
- Copyright holder:
- ESO
- Copyright date:
- 2017
- Notes:
- Copyright © 2017 ESO. Reproduced with permission from Astronomy & Astrophysics, © ESO.
Journal article
The VLT-FLAMES Tarantula Survey: XXVII. Physical parameters of B-type main-sequence binary systems in the Tarantula nebula
Actions
Access Document
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
Item Description
Terms of use
Metrics
Altmetrics
Dimensions
If you are the owner of this record, you can report an update to it here: Report update to this record