Home     Getting Started     To Survive in the Universe    
Inhabited Sky
    News@Sky     Astro Photo     The Collection     Forum     Blog New!     FAQ     Press     Login  

TYC 2945-895-1


Contents

Images

- No Images Found -
Upload your image

DSS Images   Other Images


Related articles

Four First and Two Recalculated Orbits for Binaries
In this paper, we analyze new orbital elements, and quantities that canbe derived from them, for six binaries. For four of them, WDS 00251+4803= HDS 56, WDS 01071-0036 = HDS 144 AB, WDS 06426+3955 = HDS 930, and WDS21014+4037 = HDS 2995, the orbital elements are calculated for the firsttime. For the other two, WDS 04195+3800 = HDS 552 and WDS 23209+1643 =HEI 88, the orbital elements are recalculated. Five binaries, denoted asHDS, were discovered during the Hipparcos mission while the remainingbinary was discovered somewhat earlier. HEI 88 was measured for thefirst time in 1978. All studied pairs are close, with almost allmeasured separations less than 0.3 arcsec. For these binaries theobservations were usually performed using the speckle-interferometrictechnique with the exception of HEI 88, which was observed visually oneight occasions. The resulting orbital periods fall within 13 and 69years. In addition to the orbital elements, we also give (O-C) residualsin ? and ?, masses, dynamical parallaxes, absolutemagnitudes, spectral types, and ephemerides for the next five years.

Speckle interferometry of nearby multiple stars. IV. Measurements in 2004 and new orbits
The results of speckle interferometric observations of 104 binary and 6triple stars performed at the BTA 6 m telescope in 2004 October arepresented. Nearby low-mass stars are mostly observed for the program,among which 59 there are new binaries recently discovered by theHipparcos astrometric satellite. Concurrently with thediffraction-limited position measurements we obtained 154 brightnessratio measurements of binary and multiple star components in differentbands of the visible spectrum. New, first-resolved binaries are thesymbiotic star CH Cyg with a weak companion at 0.043″ separationand the pair of red dwarfs, GJ 913 = HIP 118212. In addition, we derivedthe orbital parameters for two interferometric systems: the CN-giantpair HD 210211 = HIP 109281 (P = 10.7 yr) and the G2V-K2V G2V-K2V binaryGJ 9830 = HIP 116259 (P = 15.7 yr).

Speckle interferometry of nearby multiple stars. III.
Not Available

Submit a new article


Related links

  • - No Links Found -
Submit a new link


Member of following groups:


Observation and Astrometry data

Constellation:Ηνίοχος
Right ascension:06h42m37.43s
Declination:+39°55'12.9"
Apparent magnitude:9.253
Proper motion RA:3.7
Proper motion Dec:-20.1
B-T magnitude:10.048
V-T magnitude:9.319

Catalogs and designations:
Proper Names   (Edit)
TYCHO-2 2000TYC 2945-895-1
USNO-A2.0USNO-A2 1275-06506713
HIPHIP 32132

→ Request more catalogs and designations from VizieR