UBV photometry of IRAS 18062+2410 Virtual Observatory Resource

Authors
  1. Arkhipova V.P.
  2. Ikonnikova N.P.
  3. Noskova R.I.
  4. Sokol G.V.
  5. Esipov V.F.,Klochkova V.G.
  6. Published by
    CDS
Abstract

The photometric and spectroscopic observations of IRAS 18062+2410 = V886 Her, a candidate for protoplanetary objects, in 1996-1997 are presented. The star exhibits rapid light variations with an amplitude up to 0.3mag in V. A high-resolution spectrum of IRAS shows absorption lines of H, HeI, OI, FeII, SiII, NaI and other species, including [OII], [NII], and [FeII] that belong to the stellar envelope.

Keywords
  1. Infrared sources
  2. Planetary nebulae
  3. Optical astronomy
  4. Wide-band photometry
  5. Spectroscopy
Bibliographic source Bibcode
1999PAZh...25...30A
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/25/30
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/25/30

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/25/30
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/25/30
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/25/30
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2000-04-02T22:30:44Z
Resource record created
2000-04-02T22:30:44Z
Created
2000-04-02T22:30:47Z
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