No CrossRef data available.
Article contents
Optical spectroscopy of DPVs and the case of LP Ara
Published online by Cambridge University Press: 12 July 2011
Abstract
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.
We present preliminary results of our spectroscopic campaign of a group of intermediate mass interacting binaries dubbed “Double Periodic Variables” (DPVs), characterized by orbital light curves and additional long photometric cycles recurring roughly after 33 orbital periods (Mennickent et al. 2003, 2005). They have been interpreted as interacting, semi-detached binaries showing cycles of mass loss into the interstellar medium (Mennickent et al. 2008, Mennickent & Kołaczkowski 2009). High resolution Balmer and helium line profiles of DPVs can be interpreted in terms of mass flows in these systems. A system solution is given for LP Ara, based on modeling of the ASAS V-band orbital light curve and the radial velocity of the donor star.
Keywords
- Type
- Contributed Papers
- Information
- Copyright
- Copyright © International Astronomical Union 2011
References
Desmet, M., Frémat, Y., Baudin, F., & Harmanec, P. et al. 2010, MNRAS 401, 418CrossRefGoogle Scholar
Mennickent, R. E., Cidale, L., Díaz, M., & Pietrzyński, G. et al. 2005, MNRAS 357, 1219CrossRefGoogle Scholar
Mennickent, R. E. & Kołaczkowski, Z. 2009, Binaries: Key to Comprehension of the Universe, ASP-CS, in press, arXiv0908:3900Google Scholar
Mennickent, R. E., Kołaczkowski, Z., Michalska, G., & Pietrzyński, G. et al. 2008, MNRAS 389, 1605CrossRefGoogle Scholar
Michalska, G., Mennickent, R. E., Kołaczkowski, Z. & Djurašević, G. 2009, ASP-CS, arXiv:0910.4359Google Scholar
Svechnikov, M. A. & Kuznetsova, E. F. 1990, Katalog priblizhennykh fotometricheskikh i absoliutnykh elementov zatmennykh peremennykh zvezd (Sverdlovsk: Izd-vo Ural'skogo universiteta)Google Scholar
You have
Access