Volume 371, Number 1, May III 2001
|Page(s)||123 - 132|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||15 May 2001|
A search for peculiar objects in young open clusters*
II. A new Be star, the optical counterpart of IRAS 19564+3224 and a new open cluster in Vulpecula
Osservatorio Astronomico di Bologna, Via Ranzani 1, 40127 Bologna, Italy
2 Dipartimento de Astrofísica, Universidad de La Laguna, Avda. Astrofisico F. Sánchez sn, 30071 La Laguna, Spain
3 Istituto di Astrofisica Spaziale, CNR, Area della Ricerca di Roma Tor Vergata, V. Fosso del Cavaliere snc, 00133 Roma, Italy
Corresponding author: V. F. Polcaro, email@example.com
Accepted: 28 February 2001
A serendipitous sky field in Vulpecula was observed with Johnson BVR photometry and slitless spectroscopy in the 5600-8000 Årange, looking for emission line and late spectral type stars. We discovered that the B2V star LS II +32° 9, most probably a member of the Vul OB4 association, is now an Hα emitter. Furthermore, we identified the optical counterpart of the IRAS source IRAS 19564+3224 as a C star. Photometric study of the surrounding stellar field revealed that this object lies inside the sky area of a previously undetected open cluster of intermediate age. We discuss the possible cluster membership of the Carbon star and its implications. Some hints about the galactic structure along the line of sight of the observed field are also given
Key words: stars: carbon stars / stars: evolution / stars: emission-line, Be / stars: individual (LS II+32° 9) open clusters and associations
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.