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.

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. visible-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).