DIB in VLT-FLAMES Tarantula Survey Virtual Observatory Resource

Authors
  1. van Loon J.T.
  2. Bailey M.
  3. Tatton B.L.
  4. Maiz Apellaniz J.
  5. Crowther P.A.,de Koter A.
  6. Evans C.J.
  7. Henault-Brunet V.
  8. Howarth I.D.
  9. Richter P.,Sana H.
  10. Simon-Diaz S.
  11. Taylor W.
  12. Walborn N.R.
  13. Published by
    CDS
Abstract

The Tarantula Nebula (a.k.a. 30 Dor) is a spectacular star-forming region in the Large Magellanic Cloud (LMC), seen through gas in the Galactic disc and halo. Diffuse interstellar bands (DIBs) offer a unique probe of the diffuse, cool-warm gas in these regions. The aim is to use DIBs as diagnostics of the local interstellar conditions, whilst at the same time deriving properties of the yet-unknown carriers of these enigmatic spectral features. Spectra of over 800 early-type stars from the Very Large Telescope Flames Tarantula Survey (VFTS) were analysed. Maps were created, separately, for the Galactic and LMC absorption in the DIBs at 4428 and 6614{AA} and - in a smaller region near the central cluster R 136 - neutral sodium (the NaI D doublet); we also measured the DIBs at 5780 and 5797{AA}.

Keywords
  1. magellanic-clouds
  2. interstellar-medium
  3. line-intensities
  4. spectroscopy
Bibliographic source Bibcode
2013A&A...550A.108V
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/550/A108
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/550/A108
Document Object Identifer DOI
doi:10.26093/cds/vizier.35500108

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IVOA Cone Search SCS
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History

2013-02-04T10:48:08Z
Resource record created
2013-02-04T10:48:08Z
Created
2017-09-20T05:13:52Z
Updated

Contact

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CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr