activity
20032022
most citedRR Lyrae variables: visual and infrared luminosities, intrinsic colours, and kinematics

97 citations · 190 across the 6 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2022★ 12 cited

Search for OB associations in {\sl Gaia} early Data Release 3

Alexander A. Chemel, Richard de Grijs, Elena V. Glushkova +1

The distribution of young stars into OB associations has long been in need of updating. High-precision {\sl Gaia} early Data Release 3 astrometry, coupled with modern machine-learn…

astro-ph.GA2015★ 46 cited

Classical Cepheids and the spiral structure of the Milky Way

A. K. Dambis, L. N. Berdnikov, Yu. N. Efremov +7

We use the currently most complete collection of reliable Cepheid positions (565 stars) out to ~5 kpc based mostly on our photometric data to outline the spiral pattern of our Gala…

astro-ph.GA2014★ 33 cited

Classical Cepheids in the Galactic outer ring R1R2'

A. M. Mel'nik, P. Rautiainen, L. N. Berdnikov +2

The kinematics and distribution of classical Cepheids within ~3 kpc from the Sun suggest the existence of the outer ring R1R2' in the Galaxy. The optimum value of the solar positio…

astro-ph.GA2013★ 97 cited

RR Lyrae variables: visual and infrared luminosities, intrinsic colours, and kinematics

A. K. Dambis, L. N. Berdnikov, A. Y. Kniazev +4

We use UCAC4 proper motions and WISE W1-band apparent magnitudes intensity-mean for almost 400 field RR Lyrae variables to determine the parameters of the velocity distribution of…

astro-ph.GA2012★ 2 cited

The Baade-Becker-Wesselink technique and the fundamental astrophysical parameters of Cepheids

Alexey S. Rastorguev, Andrey K. Dambis, Marina V. Zabolotskikh +2

The BBW method remains one of most demanded tool to derive full set of Cepheid astrophysical parameters. Surface brightness version of the BBW technique was preferentially used dur…