Spectrum of bipolar nebula AFGL 2688 Virtual Observatory Resource

Authors
  1. Klochkova V.G.
  2. Szczerba R.
  3. Panchuk V.E.
  4. Published by
    CDS
Abstract

Based on echelle spectra obtained at the prime focus of the 6-m telescope, the detailed chemical composition of one of the components of the bipolar nebula identified with the intense infrared source AFGL 2688 was determined by the model-atmosphere method.

Keywords
  1. nebulae
  2. spectrophotometry
  3. line-intensities
  4. chemical-abundances
Bibliographic source Bibcode
2000PAZh...26..510K
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/26/510
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/26/510

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/26/510
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/26/510
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/26/510
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2001-05-26T20:19:42Z
Resource record created
2001-05-26T20:19:42Z
Created
2001-05-26T20:20:20Z
Updated

Contact

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