Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Nina V. Kharchenko"'
Autor:
Peter Berczik, Nina V. Kharchenko, E. S. Postnikova, Kseniia Sysoliatina, A. E. Piskunov, M. V. Ishchenko, Sabine Reffert, Evgeny Polyachenko, Dana Kovaleva, Andreas Just
Given the closeness of the two open clusters Cr 135 and UBC 7 on the sky, we investigate the possibility of the two clusters to be physically related. We aim to recover the present-day stellar membership in the open clusters Collinder 135 and UBC 7 (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2abcc0e14594877f607e80a66206e16d
http://arxiv.org/abs/2009.02223
http://arxiv.org/abs/2009.02223
Autor:
Nikolai I. Shatsky, Alexander S. Gusev, E. V. Shimanovskaya, A. E. Piskunov, Nina V. Kharchenko, F. Sakhibov
Publikováno v:
Open Astronomy, Vol 27, Iss 1, Pp 98-111 (2018)
We developed techniques for searching young unresolved star groupings (clusters, associations, and their complexes) and of estimating their physical parameters. Our study is based on spectroscopic, spectrophotometric, and UBVRI photometric observatio
Publikováno v:
Open Astronomy, Vol 26, Iss 1, Pp 219-223 (2017)
Our goal was to compare the open cluster photometric distance scale of the global survey of star clusters in the Milky Way (MWSC) with the distances derived from trigonometric parallaxes from the Gaia DR1/TGAS catalogue and to investigate to which de
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 453:1981-1989
Autor:
A. E. Piskunov, Sabine Reffert, Nina V. Kharchenko, Ralf-Dieter Scholz, S. Röser, Steffi X. Yen, Dana Kovaleva, Elena Schilbach
Publikováno v:
NASA Astrophysics Data System
The global survey of star clusters in the Milky Way (MWSC) is a comprehensive list of 3061 objects that provides, among other parameters, distances to clusters based on isochrone fitting. The Tycho-Gaia Astrometric Solution (TGAS) catalogue, which is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e47a09282c52bc81e1e3c1f0cb8295a
http://arxiv.org/abs/1709.09975
http://arxiv.org/abs/1709.09975
Autor:
Steffi X. Yen, Siegfried Röser, Sabine Reffert, Elena Schilbach, A. E. Piskunov, Nina V. Kharchenko
Publikováno v:
Proceedings of the International Astronomical Union. 12:281-282
We have developed a fully automated cluster characterization pipeline, which simultaneously determines cluster membership and fits the fundamental cluster parameters: distance, reddening, and age. We present results for 24 established clusters and co
Autor:
Siegfried Röser, A. E. Piskunov, Nina V. Kharchenko, Ralf-Dieter Scholz, Elena Schilbach, Hans Zinnecker
Publikováno v:
Reviews in Modern Astronomy: Deciphering the Universe through Spectroscopy, Volume 22
It is textbook knowledge that open clusters are conspicuous members of the thin disk of our Galaxy, but their role as contributors to the stellar population of the disk was regarded as minor. Starting from a homogenous stellar sky survey, the ASCC-2.
Publikováno v:
Astronomy & Astrophysics. 507:L5-L8
(...) We search for an explanation of the disagreement between the observed integrated colours of 650 local Galactic clusters and the theoretical colours of present-day SSP models. We check the hypothesis that the systematic offsets between observed
Autor:
Hans Zinnecker, A. E. Piskunov, Elena Schilbach, R.-D. Scholz, Nina V. Kharchenko, Siegfried Röser
Publikováno v:
Astronomy & Astrophysics. 504:681-688
Aims. We determine the integrated magnitudes and colours of 650 clusters in optical (BV) and the near-infrared (JHKs) passbands and construct the luminosity functions of the Galactic open clusters in these passbands. Methods. The magnitudes are based
Autor:
A. E. Piskunov, Nina V. Kharchenko, Peter Berczik, R.-D. Scholz, S. Röser, M. I. Petrov, Elena Schilbach
Publikováno v:
Astronomy & Astrophysics. 495:807-818
(abridged) In this paper we derive observed and modelled shape parameters (apparent ellipticity and orientation of the ellipse) of 650 Galactic open clusters identified in the ASCC-2.5 catalogue. We provide the observed shape parameters of Galactic o