14,307 datasets found

Keywords: stellar astronomy

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  • Orientation of orbits in triple stars

    A sample of visual syb-systems from the Multiple Star Catalog (Tokovinin, 1997, Cat. ) is selected where the apparent sense of rotation (prograde or retrograde) at two adjacent...
  • Long-period companions of multiple stars

    We examined the statistics of an angle gamma between the radius vector of a visual companion of a multiple star and the vector of its apparent relative motion in the system. We...
  • CCD measurements of double stars

    We present measurements of visual double stars made by CCD imaging from 1996 to 1999. In the article, Table 1 contains the measurements of 51 binaries with known orbit. The...
  • Ap stars periodicity

    New data on the periods of Ap stars with references are presented. 161 further stars are introduced for which a periodic variability has recently been discovered or it was known...
  • SV Cam BVR light curves

    New BVR light curves and times of minimum light for the short period RS CVn system SV Cam were analysed to derive the physical parameters of the system and the parameters of the...
  • Photometry in NGC 2516

    We present the results of a 0.86 square degree CCD photometric survey of the open cluster NGC 2516, which has an age of about 150Myr and may have a much lower metallicity than...
  • Monoperiodic pulsating stars in the OGLE database

    Files table3, table4, table5 contain the parameters of the Fourier fits of the light curves of monoperiodic OGLE variables with P<1d (High-Amplitude {delta} Scuti (HADS), RRc...
  • Empirical relations for cluster RR Lyrae

    Our former study on the empirical relations between the Fourier parameters of the light curves of the fundamental mode RR Lyrae stars and their basic stellar parameters has been...
  • OB associations in the spiral galaxy NGC 300

    We present results of a search for OB associations in NGC 300. Using an automatic and objective method (PLC technique) 117 objects were found. Statistical tests indicate that...
  • UVKs photometry of globular clusters in NGC 5128

    At the distance of NGC 5128 (3.6+/-0.2Mpc) it is possible to resolve globular clusters with high resolution imaging from the ground, thus allowing the globular cluster candidate...
  • Double stars measurements at Nice Obs.

    We present (table 1) the measurements of 58 visual double stars made in 1999 and 2000 with the 50 cm refractor of the Nice Observatory and attached CCD camera, using an...
  • T Tauri binary systems orbital motion

    Using speckle-interferometry we have carried out repeated measurements of relative positions for the components of 34 T Tauri binary systems. The projected separation of these...
  • Reddening in open and globular clusters

    This paper compares reddening values E(B-V) derived from the stellar content of 103 old open clusters and 147 globular clusters of the Milky Way with those derived from...
  • Lindroos binary systems X-ray emission

    We present a study of the X-ray emission from binary systems extracted from the Lindroos catalogue (Lindroos, 1986A&A...156..223L) based on the ROSAT All-Sky survey as well...
  • TZ Boo & Y Sex orbital periods

    TZ Boo and Y Sex are two A-type contact binaries. At the set, times of light minimum of the two stars were collected.
  • DL Cygni ubr differential photometry

    Relative photometry of DL Cygni versus GSC 3595-0200 in the instrumental system
  • Imaging of symbiotic stars

    Narrowband images of 51 symbiotic stars were obtained at the ESO and ORM observatories to search for resolved optical nebulae. Ionized nebulae much larger than previously known...
  • HST photometry of ESO 338-IG04 globular clusters

    Multicolour images of the starbursting metal poor blue compact galaxy ESO 338-IG04 have been obtained with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope....
  • Limb-darkening coefficients for ubvyUBVRIJHK

    Linear and non-linear limb-darkening coefficients for the photometric bands u v b y U B V R I J H K are computed for very low effective temperatures stars. The atmosphere models...
  • Be stars variability

    The high accuracy and the homogeneity of Hipparcos data for bright stars have allowed us to quantify the degree of variability of Be stars. This degree has been found to be...
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