VR + velocity variations of IRAS 11472-0800

DOI

We focus here on one particular and poorly studied object, IRAS 11472-0800. It is a highly evolved post-asymptotic giant branch (post-AGB) star of spectral type F, with a large infrared excess produced by thermal emission of circumstellar dust. We deployed a multi-wavelength study that includes the analyses of optical and IR spectra as well as a variability study based on photometric and spectroscopic time-series.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35420053
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/542/A53
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A53
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A53
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/542/A53
Provenance
Creator Van Winckel H.; Hrivnak B.J.; Gorlova N.; Gielen C.; Lu W.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Exoplanet Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy