International audienceContext: BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very complex frequency spectrum is detected, with a number of independent nonradial modes excited, unusual among the high-amplitude pulsators in the Lower Classical Instability Strip. Aims: An extensive and detailed study has been carried out to investigate the pulsational content and properties of this object. Methods: The analysis is based on 283 h of CCD observations obtained in the Johnson V filter, during a long multisite photometric campaign carried out along the Northern autumn-winter of 2005-2006. Additionally, multicolour BI photometry was also collected to study the phase shifts and amplitude ratios, between light ...
International audienceContext: HD 181231 is a B5IVe star, which has been observed with the CoRoT sat...
International audienceContext: Solar-like oscillations have been discovered in a few red giants, inc...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...
International audienceContext: BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
WOS: 000248394400032Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type v...
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Ph...
Context.Short-period high-amplitude pulsating stars of Population I (d Sct stars) and II (SX Phe var...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
Context. Short-period high-amplitude pulsating stars of Population I (δ Sct stars) and II (SX Phe v...
Astronomy and Astrophysics, v. 451, p. 999-1008, 2006. http://dx.doi.org/10.1051/0004-6361:20053841I...
Contains fulltext : 34555.pdf (publisher's version ) (Open Access)Aims. We selecte...
International audienceContext: HD 181231 is a B5IVe star, which has been observed with the CoRoT sat...
International audienceContext: Solar-like oscillations have been discovered in a few red giants, inc...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...
International audienceContext: BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
WOS: 000248394400032Context. BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type v...
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
Context. Short-period high-amplitude pulsating stars of Population I (delta Sct stars) and II (SX Ph...
Context.Short-period high-amplitude pulsating stars of Population I (d Sct stars) and II (SX Phe var...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
Context. Short-period high-amplitude pulsating stars of Population I (δ Sct stars) and II (SX Phe v...
Astronomy and Astrophysics, v. 451, p. 999-1008, 2006. http://dx.doi.org/10.1051/0004-6361:20053841I...
Contains fulltext : 34555.pdf (publisher's version ) (Open Access)Aims. We selecte...
International audienceContext: HD 181231 is a B5IVe star, which has been observed with the CoRoT sat...
International audienceContext: Solar-like oscillations have been discovered in a few red giants, inc...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...