Zobrazeno 1 - 10
of 50
pro vyhledávání: '"Vakhtang S. Tamazian"'
Autor:
Manuel Andrade, R. Carini, Enzo Brocato, Luca Piccotti, José A. Docobo, Vakhtang S. Tamazian, P. P. Campo
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:2709-2721
The study of a selected set of 69 double-lined spectroscopic binaries (SB2) with well-defined visual and spectroscopic orbits was carried out. The orbital parallax, the mass, the colour, and the luminosity of each component were derived from observat
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 476:2792-2800
In the vast majority of cases when available astrometric measurements of a visual binary cover a very short orbital arc, it is practically impossible to calculate a good quality orbit. It is especially important for systems with pre-main-sequence com
Autor:
Marco Scardia, Brian D. Mason, Vakhtang S. Tamazian, Bo Reipurth, Andrei Tokovinin, T. ten Brummelaar, Frédéric Arenou, Patricia Lampens, Yuri Balega, José A. Docobo
Publikováno v:
Proceedings of the International Astronomical Union. 11:388-412
This report covers the workings of Commission 26 over the triennial period 2012-2015 and is the last report of the Commission. Included are reports from Working Groups and the Commission 26 Circular; all of which will be continuing in Commission G1 (
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 444:3641-3646
We report a comprehensive study of the binary system COU 2031, based on simultaneous and independent astrometric visual and speckle observations and on radial-velocity measurements. The similarity of the two orbital solutions allows us to obtain not
Publikováno v:
Astrophysics. 56:8-18
Results of spectral monitoring of the flare stars HU Del, CM Dra, WX UMa, and VW Com by the 2.6-m telescope at the Byurakan Observatory during May-June 2012 with the SCORPIO spectral camera are reported. A strong flare of WX UMa was recorded during t
Improved orbits are presented for the visual binaries WDS 02366+1227, WDS 02434-6643, WDS 03244-1539, WDS 08507+1800, WDS 09128-6055, WDS 11532-1540, WDS 17375+2419, and WDS 22408-0333. The latest orbits for these binaries were demonstrating a great
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f3c123cf756d262692428310434dc31
http://arxiv.org/abs/1609.03392
http://arxiv.org/abs/1609.03392
Publikováno v:
Astrophysics. 54:469-475
This is an analysis of the dependence of the flare activity of the well known flare star UV Ceti on the linear distance between the components of this binary system. It is shown that its flaring activity clearly depends on the mutual distance of the
Publikováno v:
Astrophysics. 54:377-383
A continued search for emission objects in three new fields within the association Cyg OB7 yielded eight new emission stars in one of these fields. No emission stars were detected in the other two fields, apparently because we have come to the bounda
Publikováno v:
Astrophysics. 54:203-213
A search for Hα objects in four fields with an overall area of about 0.14 square degrees in the region of NGC 6910 (the core of the known Cyg OB9 association) has led to the discovery of 64 emission stars, of which 49 are newly detected. The high su
Publikováno v:
The Astronomical Journal. 140:1078-1083
Results of the EMCCD-based speckle interferometric observations and differential photometry for 46 visual binaries obtained in 2007 June and July with the 6 m telescope of the Special Astrophysical Observatory (Russia) are presented. First preliminar