The UVES Paranal Observatory Project Spectrum Preview Interface

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S. Bagnulo, R. Cabanac, E. Jehin, C. Ledoux, C. Melo,

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UVES POP tables: IC 2391 - NGC 6475 - Field Stars - Brightest Stars

Return to UVES SPI for new search

Choose your favorite POP star

Select one of the available stars from the scroll down menu (single plot)

List of available POP stars

Or search in the database using the searching boxes to overplot up to five stars on the same plot
NB: The search tool is not intended to allow users to perform complex searches. In particular, be aware that the strings I, *I, and I* are strictly equivalent to the string *I* for the search algorithm. In addition space, comma and semi-colon characters are all interpreted as separators for name search.

Pecularities should be chosen among the following (NB case sensitive!):
agb asymptotic giant branch star, c carbon star ceph cepheid cl member of a cluster d double/multiple el shows emission lines ebAgl eclipsing binary of Algol type ev ellipsoidal variable f O star with He and NIII emission G-CN G and CN-Band He-s helium strong He-w helium weak hpm high proper motion m magnetic MetA metallic A Star mp metal poor n diffuse line pagb post-asympotic giant branch star pv pulsating variable S S star sb Spectroscopic binary Si Eu Sr Cr Fe (or any element) Si, Eu, Sr, Cr, Fe (or any element) strong star she shell v used when SIMBAD defines a star as variable without specifying the variability type, otherwise we use the variability type instead of v. List of abbreviated variability types used in the tables bCep Beta Cephi variable BYDra BY Draconis variable dSct delta Scuti variable MirCet Mira Ceti variable nova nova rsCVn RS Canes Venatici variable srp Semi-Regular Pulsating variable wr Wolf-Rayet star
(See legend page)