Emission lines of Sr filament near {eta} Car Virtual Observatory Resource

Authors

1. Hartman H.
2. Gull T.
3. Johansson S.
4. Smith N.,HST Eta Carinae Treasury Project Team

Published by

CDS

Abstract

We have obtained deep spectra from 1640 to 10100{AA} with the Space Telescope Imaging Spectrograph (STIS) of the strontium filament, a largely neutral emission nebulosity lying close to the very luminous star Eta Carinae and showing an uncommon spectrum. Over 600 emission lines, both permitted and forbidden, have been identified.

Keywords

1. variable-stars
2. spectroscopy
3. ultraviolet-astronomy

Bibliographic source Bibcode

2004A&A...419..215H

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/419/215

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/419/215

Document Object Identifer DOI

doi:10.26093/cds/vizier.34190215

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/419/215
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/419/215
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/419/215

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).