The pulsation activity of small-amplitude Cepheid Alpha UMi (Polaris) during the period of its radial velocity observations has been analyzed. In the 20th century, Polaris was known to demonstrate a decrease in radial velocity amplitude to the minimum, in the 1980s. Thereafter, the amplitude has increased. The observations of September-December 2015 (21 spectra) obtained by 81cm telescope TCO with spectrograph have showed that radial velocity amplitude comes to 4.16 km/s and is approximately twice higher than the estimates made in 2007, with pulsation period adding 8.6 min
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
A digital parallel processor has been constructed for use with a wide-band polarimeter. The process...
The pulsation activity of small-amplitude Cepheid Alpha UMi (Polaris) during the period of its radia...
Abstract. We present recent results of precise radial velocity measurements of Po-laris collected du...
We present the results of an analysis of 21 spectra of alpha UMi (Polaris) obtained in September – D...
We investigate temporally changing variability amplitudes and the multi-periodicity of the type-I Ce...
Presented herein are preliminary radial velocity results for two classical Cepheids: V440 Per and α ...
We present the results of the radial velocity (RV ) measurements of metallic lines as well as Hα (H...
A recently presented HST/FGS parallax measurement of the Polaris system has been interpreted as evid...
Measurements of secular period change probe real-time stellar evolution of classical Cepheids making...
Context. Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic ...
We present the results of our analysis of high-resolution spectroscopic observations of Cepheid α UM...
Context. The dependence of amplitude on the pulsation period differs from other Cepheid-related re...
15 pages, 3 postscript figures, accepted for publication on ApJ LettersWe present new theoretical Pe...
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
A digital parallel processor has been constructed for use with a wide-band polarimeter. The process...
The pulsation activity of small-amplitude Cepheid Alpha UMi (Polaris) during the period of its radia...
Abstract. We present recent results of precise radial velocity measurements of Po-laris collected du...
We present the results of an analysis of 21 spectra of alpha UMi (Polaris) obtained in September – D...
We investigate temporally changing variability amplitudes and the multi-periodicity of the type-I Ce...
Presented herein are preliminary radial velocity results for two classical Cepheids: V440 Per and α ...
We present the results of the radial velocity (RV ) measurements of metallic lines as well as Hα (H...
A recently presented HST/FGS parallax measurement of the Polaris system has been interpreted as evid...
Measurements of secular period change probe real-time stellar evolution of classical Cepheids making...
Context. Classical Cepheids (DCEPs) are the most important primary indicators for the extragalactic ...
We present the results of our analysis of high-resolution spectroscopic observations of Cepheid α UM...
Context. The dependence of amplitude on the pulsation period differs from other Cepheid-related re...
15 pages, 3 postscript figures, accepted for publication on ApJ LettersWe present new theoretical Pe...
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
Polaris the Cepheid has been observed for centuries, presenting surprises and changing our view of C...
A digital parallel processor has been constructed for use with a wide-band polarimeter. The process...