Astronomy and Astrophysics, v. 451, p. 999-1008, 2006. http://dx.doi.org/10.1051/0004-6361:20053841International audienc
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Abstract CO Cam (TIC 160268882) is the second “single-sided pulsator” to be discovered. These are st...
BM Camelopardalis (=12 Cam) is a chromospherically active binary star with a relatively large orbita...
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 (d Sct stars) and II (SX Phe var...
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 (δ Sct stars) and II (SX Phe v...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
A spectroscopic and photometric analysis has been carried out for 32 candidate SX Phe variable blue ...
We present a study of the high-resolution (R = 60 000) optical spectrum of the B[e] supergiant CI Ca...
Context. The Galactic supergiant B[e] star CI Camelopardalis (CI Cam) was the first sgB[e] star dete...
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Abstract CO Cam (TIC 160268882) is the second “single-sided pulsator” to be discovered. These are st...
BM Camelopardalis (=12 Cam) is a chromospherically active binary star with a relatively large orbita...
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 (d Sct stars) and II (SX Phe var...
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 (δ Sct stars) and II (SX Phe v...
Context. BL Cam is an extreme field multiperiodic short-period low-metallicity high-amplitude SX Phe...
A spectroscopic and photometric analysis has been carried out for 32 candidate SX Phe variable blue ...
We present a study of the high-resolution (R = 60 000) optical spectrum of the B[e] supergiant CI Ca...
Context. The Galactic supergiant B[e] star CI Camelopardalis (CI Cam) was the first sgB[e] star dete...
Context.BL Cam is an extreme metal-deficient field high-amplitude SX Phe-type variable where a very...
Abstract CO Cam (TIC 160268882) is the second “single-sided pulsator” to be discovered. These are st...
BM Camelopardalis (=12 Cam) is a chromospherically active binary star with a relatively large orbita...
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