Abstract. In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper presents the results including one new roAp star (HD 122970), the con rmation of rapid oscillations of HD 99563 and appar-ent null results for other stars. Using Hipparcos data a statistical analysis of the ab-solute magnitudes and galactic distributions of all known roAp and noAp stars (also taken from the literature) was made. A systematic trend for most of the program stars in a MV vs. (index of the Strömgren uvby system) dia-gram was detected leading to the conclusion that is sys-tematically influenced by the chemical peculiarity and/or magnetic eld. Three roAp stars are outside the Scuti instability strip which implies that the ...
Context. Rapidly oscillating Ap (roAp) stars have rarely been found in binary or higher order multi...
Context. The rapidly oscillating Ap (roAp) stars exhibit short time scale photometric and/or radial ...
Abstract. The search of roAp stars at Mt. Dushak–Erekdag Observatory was started in 1992 using the 0...
In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper prese...
Abstract. The Naini Tal-Cape survey has been initiated to search for pul-sations in chemically pecul...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
Abstract. This paper reviews some of the important advances made over the last decade concerning the...
Context. Chemically peculiar Ap stars are main-sequence stars of spectral type B8–F3 which show larg...
To reliably determine the spectroscopic signature of rapidly oscillating chemically peculiar (roAp) ...
Context. Chemically peculiar Ap stars are main-sequence stars of spectral type B8–F3 which show larg...
To reliably determine the spectroscopic signature of rapidly oscillating chemically peculiar (roAp) ...
Context. Rapidly oscillating Ap (roAp) stars have rarely been found in binary or higher order multi...
Context. The rapidly oscillating Ap (roAp) stars exhibit short time scale photometric and/or radial ...
Abstract. The search of roAp stars at Mt. Dushak–Erekdag Observatory was started in 1992 using the 0...
In 1995 we initiated a Northern Hemisphere survey for rapidly oscillating Ap stars. This paper prese...
Abstract. The Naini Tal-Cape survey has been initiated to search for pul-sations in chemically pecul...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
Chemically peculiar stars are stage to a wide variety of physical phenomena, including diffusion, co...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
The rapidly oscillating Ap (roAp) stars are cool, magnetic, chemically peculiar stars which pulsate ...
Abstract. This paper reviews some of the important advances made over the last decade concerning the...
Context. Chemically peculiar Ap stars are main-sequence stars of spectral type B8–F3 which show larg...
To reliably determine the spectroscopic signature of rapidly oscillating chemically peculiar (roAp) ...
Context. Chemically peculiar Ap stars are main-sequence stars of spectral type B8–F3 which show larg...
To reliably determine the spectroscopic signature of rapidly oscillating chemically peculiar (roAp) ...
Context. Rapidly oscillating Ap (roAp) stars have rarely been found in binary or higher order multi...
Context. The rapidly oscillating Ap (roAp) stars exhibit short time scale photometric and/or radial ...
Abstract. The search of roAp stars at Mt. Dushak–Erekdag Observatory was started in 1992 using the 0...