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3D stellar reddening map from 2MASS photometry: An improved version
DOI: 10.1134/S1063773717070039 Bibcode: 2017AstL...43..472G

Gontcharov, G. A.

An improved version of the 3D stellar reddening map in a space with a radius of 1200 pc around the Sun and within 600 pc of the Galactic midplane is presented. As in the previous 2010 and 2012 versions of the map, photometry with an accuracy better than 0.05 m in the J and Ks bands for more than 70 million stars from the 2MASS catalogu…

2017 Astronomy Letters
Gaia 48
Kinematics of the galaxy from OB stars with proper motions from the Gaia DR1 catalogue
DOI: 10.1134/S1063773717030021 Bibcode: 2017AstL...43..159B

Bobylev, V. V.; Bajkova, A. T.

We consider two samples of OB stars with different distance scales that we have studied previously. The first and second samples consist of massive spectroscopic binaries with photometric distances and distances determined from interstellar calcium lines, respectively. The OB stars are located at heliocentric distances up to 7 kpc. We have identif…

2017 Astronomy Letters
Gaia 22
Kinematics of the galaxy from Cepheids with proper motions from the Gaia DR1 catalogue
DOI: 10.1134/S106377371703001X Bibcode: 2017AstL...43..152B

Bobylev, V. V.

A sample of classical Cepheids with known distances and line-of-sight velocities has been supplemented with proper motions from the Gaia DR1 catalogue. Based on the velocities of 260 stars, we have found the components of the peculiar solar velocity vector ( U, V, W) = (7.90, 11.73, 7.39) ± (0.65, 0.77, 0.62) km s-1 and the …

2017 Astronomy Letters
Gaia 21
Systematic error of the Gaia DR1 TGAS parallaxes from data for the red giant clump
DOI: 10.1134/S1063773717060044 Bibcode: 2017AstL...43..545G

Gontcharov, G. A.

Based on the Gaia DR1 TGAS parallaxes and photometry from the Tycho-2, Gaia, 2MASS, andWISE catalogues, we have produced a sample of 100 000 clump red giants within 800 pc of the Sun. The systematic variations of the mode of their absolute magnitude as a function of the distance, magnitude, and other parameters have been analyzed. We show that the…

2017 Astronomy Letters
Gaia Hipparcos 13
Searching for stars closely encountering with the solar system based on data from the Gaia DR1 and RAVE5 catalogues
DOI: 10.1134/S1063773717080011 Bibcode: 2017AstL...43..559B

Bobylev, V. V.; Bajkova, A. T.

We have searched for the stars that either encountered in the past or will encounter in the future with the Solar system closer than 2 pc. For this purpose, we took more than 216 000 stars with the measured proper motions and trigonometric parallaxes from the Gaia DR1 catalogue and their radial velocities from the RAVE5 catalogue. We have found se…

2017 Astronomy Letters
Gaia 13
Vertical distribution and kinematics of planetary nebulae in the milky way
DOI: 10.1134/S1063773717040028 Bibcode: 2017AstL...43..304B

Bobylev, V. V.; Bajkova, A. T.

Based on published data, we have produced a sample of planetary nebulae (PNe) that is complete within 2 kpc of the Sun. We have estimated the total number of PNe in the Galaxy from this sample to be 17 000±3000 and determined the vertical scale height of the thin disk based on an exponential density distribution to be 197 ± 10 pc. The next sample …

2017 Astronomy Letters
Gaia 5
Properties of the Tycho-2 catalogue from Gaia data release
DOI: 10.1134/S106377371711007X Bibcode: 2017AstL...43..730V

Tsvetkov, A. S.; Vityazev, V. V.; Petrov, S. D. +2 more

Based on the measurements performed in the first 14 months of Gaia operation, we have solved the problem of obtaining the systematic differences between the stellar positions and proper motions of the TGAS (Tycho-Gaia Astrometric Solution) and Tycho-2 catalogues. By dividing the common stars from the TGAS and Tycho-2 catalogues into three G-magnit…

2017 Astronomy Letters
Gaia Hipparcos 4
Vertical distribution and kinematics of protoplanetary nebulae in the galaxy
DOI: 10.1134/S1063773717070027 Bibcode: 2017AstL...43..452B

Bobylev, V. V.; Bajkova, A. T.

The catalogue of protoplanetary nebulae by Vickers et al. has been supplemented with the line-of-sight velocities and proper motions of their central stars from the literature. Based on an exponential density distribution, we have estimated the vertical scale height from objects with an age less than 3 Gyr belonging to the Galactic thin disk (lumi…

2017 Astronomy Letters
Gaia 4