No CrossRef data available.
Article contents
Do the Pre-Main Sequence δ Scuti Stars Really Exist?
Published online by Cambridge University Press: 12 April 2016
Extract
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
Recently, new views of the current status of δ Scuti stars have been developed by Rodríguez & Breger (2001) who carried out an excellent review, listing 8 pre-main-sequence (PMS) δ Scuti candidates and examined the possibility of the existence of PMS δ Scuti variable stars. Here we discuss the nature of 4 stars from their list: 2 said to be members of NGC 2264 and 2 of NGC 6823.
- Type
- Part 2.4. Delta Scuti Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
References
Kurtz, D.W.
2000, in ASP Conf. Ser., Vol. 210, Delta Scuti and Related Stars, eds. Breger, M. & Montgomery, M., (San Francisco ASP), 287
Google Scholar
Peña, J.H., Peniche, R., Cervantes, F., Garcia, R., & Sareyan, J.P.
2000, ASP Conf. Ser., Vol. 203, The Impact of Large Scale Surveys on Variable Star Research, eds. Szabados, L. & Kurtz, D., (San Francisco ASP), 465
Google Scholar
You have
Access