Twenty magnetic Chemically Peculiar (CP2) stars of the SrCrEu subgroup mostly brighter than the 7.5 visual magnitude have been investigated in the near infrared at 1.25, 1.6 and 2.2 μ. The stars HD 3980, HD 24712, HD 49976, HD 83368, HD 96616, HD 98088, HD 118022, HD 125248, HD 148898, HD 203006, and HD 220825 have been found to be variable in the infrared with the same period as the visible light, spectrum, and magnetic field variations. HD 221760 is also variable with a period of 12.45 days, which has to be confirmed. The stars HD 72968, HD 111133, HD 126515, HD 153882, and HD 164258 do show some hint of variability, although the data are too few. Infrared variability has been detected for the first time in the stars HD 101065, ...
Abstract. Photoelectric photometry of 803 southern BS objects in the a-system as detection tool for ...
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
Context. Although photometric variations of chemically peculiar (CP) stars are frequently used to d...
Twelve magnetic Chemically Peculiar (CP2) stars of the SiSrCrEu subgroup mostly brighter than the 7...
Abstract. Twenty magnetic Chemically Peculiar (CP2) stars of the SrCrEu subgroup mostly brighter tha...
Context. The chemically peculiar (CP) stars of the upper main sequence are well suited for investiga...
About 10 per cent of upper main-sequence stars are characterized by the presence of chemical peculia...
The Hipparcos photometry of the Chemically Peculiar main sequence B, A, and F stars is examined fo...
The aim of this work is to study the capacity of the $uvby H_{\beta}$ system for detecting the chemi...
We aim to carry out a study on the photometric and spectroscopic variabilities of four stars monitor...
For a sample of chemically peculiar stars, we report time-resolved measurements of the effective mag...
This paper presents new near infrared observations of 160 Irregular variables of type Lb in the $JH...
Context. Chemically peculiar stars of the upper part of the main sequence show periodical variabilit...
We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemi...
We present the results of a near-infrared monitoring programme of a selected sample of stars, initia...
Abstract. Photoelectric photometry of 803 southern BS objects in the a-system as detection tool for ...
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
Context. Although photometric variations of chemically peculiar (CP) stars are frequently used to d...
Twelve magnetic Chemically Peculiar (CP2) stars of the SiSrCrEu subgroup mostly brighter than the 7...
Abstract. Twenty magnetic Chemically Peculiar (CP2) stars of the SrCrEu subgroup mostly brighter tha...
Context. The chemically peculiar (CP) stars of the upper main sequence are well suited for investiga...
About 10 per cent of upper main-sequence stars are characterized by the presence of chemical peculia...
The Hipparcos photometry of the Chemically Peculiar main sequence B, A, and F stars is examined fo...
The aim of this work is to study the capacity of the $uvby H_{\beta}$ system for detecting the chemi...
We aim to carry out a study on the photometric and spectroscopic variabilities of four stars monitor...
For a sample of chemically peculiar stars, we report time-resolved measurements of the effective mag...
This paper presents new near infrared observations of 160 Irregular variables of type Lb in the $JH...
Context. Chemically peculiar stars of the upper part of the main sequence show periodical variabilit...
We have analysed the photometric data obtained with the STEREO spacecraft for 558 non-magnetic chemi...
We present the results of a near-infrared monitoring programme of a selected sample of stars, initia...
Abstract. Photoelectric photometry of 803 southern BS objects in the a-system as detection tool for ...
Context. The (magnetic) chemically peculiar (CP) stars of the upper main sequence are well-suited la...
Context. Although photometric variations of chemically peculiar (CP) stars are frequently used to d...