Context. 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 curves obtained in dif...
International audienceContext: To understand the origin of stellar activity in pre-main-sequence Her...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...
International audienceAims:We present accurate photometric time series of two Be stars: NW Ser and V...
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...
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. 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...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
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...
Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis ...
Contains fulltext : 34555.pdf (publisher's version ) (Open Access)Aims. We selecte...
International audienceContext: To understand the origin of stellar activity in pre-main-sequence Her...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...
International audienceAims:We present accurate photometric time series of two Be stars: NW Ser and V...
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...
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. 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...
International audienceContext. Short-period high-amplitude pulsating stars of Population I (delta Sc...
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...
Differential time-series observations of BL Camelopardalis classified as a double mode SX Phoenicis ...
Contains fulltext : 34555.pdf (publisher's version ) (Open Access)Aims. We selecte...
International audienceContext: To understand the origin of stellar activity in pre-main-sequence Her...
Extensive photometric multisite campaigns of the δ Scuti variable FG Vir are presented. For the year...
International audienceAims:We present accurate photometric time series of two Be stars: NW Ser and V...