V1119 Tauri
catalogues and names
catalogues and names | V1119 Tau, 111 Tau, HR 1780, HD 35296, SAO 94526, BD +17 920, WDS 05244+1723A |
constellation | Taurus |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 5h 24min 25.4sec | DEC: +17° 23' 0'' | ||
position (B1900) | RA: 5h 18min 35.2sec | DEC: +17° 17' 26'' | ||
proper motion (J2000) | RA: 0.246 arcsec/a | DEC: -0.009 arcsec/a | ||
radial velocity | 37 km/s note: spectroscopic binaries |
|||
rotational velocity | 16 km/s (uncertain) (variable) | |||
trigonometric parallax | 0.067 arcsec | |||
galactic coordinates | longitude: 187.2° | latitude: -10.29° |
magnitude
visual magnitude | 4.99 (V on UBV Johnson system) |
spectral / color information
spectral class | F8V |
B-V-magnitude | 0.53 |
U-B-magnitude | -0.07 |
double/multiple star system information
separation | 85.7 arcsec |
mag difference (of double or brightest multiple) | 2.9 |
note | Worley (1978) update of the IDS |
note (category: double and multiple data): | Companion optical. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 5h 24min 25.421sec | DEC: +17° 23' 0.7'' | ±0.2 arcsec | source: 52 |
proper motion (J2000) | RA: 0.0165 arcsec/a | DEC: -0.009 arcsec/a | source: 25 | |
radial velocity | 37 km/s | source: 25 | ||
trigonometric parallax | 0.067 arcsec | ±0.007 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 187.2° | latitude: -10.29° |
magnitude:
visual | 4.99 (observed) | source: 25 |
photovisual | 5.1 | source: 2 |
photographic | 5.5 | source: 16 |
spectral information:
spectral class | G0 | source: 96 | |
Morgan-Keenan | F8V | source: 25 | |
B-magnitude | 5.52 ±0.05 | B-V-magnitude | 0.53 |
U-magnitude | 5.45 ±0.05 | U-B-magnitude | -0.07 |
double/multiple star system information:
separation between brightest and second brightest component | 85.4 arcsec |
magnitude difference between brightest and second brightest component | 4 |
position angle | 271 ° |
component | magnitude | spectral class | catalogue(s)/name(s) |
A | 4.99 | G0 | 111 Tau, HR 1780, HD 35296, SAO 94526 |
B | 8.37 | K0 |
sources:
2 | HD and HDE Catalogs |
Cannon, A.J., and E.C. Pickering, Harvard Annals, Vols 91-99, 1918-24, Cambridge, Massachusetts: Harvard University; Cannon, A.J., Harvard Annals, Vol. 100, 1925-36, Cambridge, Massachusetts: Harvard University; and Cannon, A.J., and M. Walton Mayall, Harvard Annals, Vol. 112, 1949, Cambridge, Massachusetts: Harvard University | |
16 | PPM North and PPM South Catalogs and PPM Supplement |
Roser, S., and U. Bastian, "Catalogue of Positions and Proper Motions," A&AS, Vol. 74, p. 449, 1988, and Bastian, U., et al., "Catalogue of Positions and Proper Motions - South," 1993 | |
19 | WDS Catalog |
Worley, C.E., and G.G. Douglass, Washington Catalog of Visual Double Stars 1996.0, United States Naval Observatory, 1996 | |
25 | Bright Star Catalogue, 5th edition |
Hoffleit, D. and Warren, W.H. Jr., The Bright Star Catalogue, 5th Revised Edition, Version 2, 1994 | |
52 | PPMN-HP subset |
PPMN Star Catalogue (Reference 16) High-Precision Subset (Code H) | |
96 | SAO or HD/HDE Catalog |
Reference from Value 1 or Reference from Value 2 |
data from Smithsonian Astrophysical Observatory Star Catalog (SAO Staff 1966; USNO, ADC 1990)
position and proper motion:
position (B1950) | RA: 5h 21min 30.232sec | DEC: +17° 20' 19.58'' | ±0.017 arcsec |
position (J2000) | RA: 5h 24min 25.446sec | DEC: +17° 23' 0.44'' | |
proper motion B1950 (FK4) | RA: 0.0172 arcsec/a | DEC: -0.008 arcsec/a | ±0.003 arcsec/a in RA ±0.002 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0.0172 arcsec/a | DEC: -0.009 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 5.1 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | G0 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | GC, catalogue number: 6645 |
Durchmusterung | BD+17 920 |
Boss General Catalogue | 6645 |
Henry Draper Catalogue | 35296 |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 5h 24.4min | DEC: +17° 23' |
proper motion (J2000) | RA: 0.249 arcsec/a | DEC: -0.005 arcsec/a |
double/multiple star system information:
component | year | number of measures | position angle | angular separation | magnitude of 1st component | magnitude of 2nd component | spectral class(es) | discoverer code |
- | 1825 | 13 | 271° | 61.8'' | 4.99 | 9 | F8V | S 478 |
1922 | - | 85.4'' |
discoverer information:
discoverer code | discoverer | reference |
S 478 | South, J. | - |
notes:
note | 111 Tau. A is a spectroscopic binary. B is BD+17@919. Proper motion of B +027 -019. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 5h 21min 30.3sec | DEC: +17° 20' 20'' |
variability informations:
variability type | BY | rotating variable star |
magnitute at max. brightness | 4.98 | |
magnitute at min. brightness | 5.02 | |
photometric system | visual, photovisual or Johnson's V |
references
to a study | K.Stepien, E.Geyer, AsAp Suppl 117, No.1, 83, 1996. |
to a chart/photograph |
miscanellous
ID in the GCVS catalogue | 78/1119 |
constellation | Taurus |
notes on existence | The star is equivalent to '73152'. |
variability type description
variability type | description |
BY | BY Draconis-type variables, which are emission-line dwarfs of dKe-dMe spectral type showing quasiperiodic light changes with periods from a fraction of a day to 120 days and amplitudes from several hundredths to 0.5 mag in V. The light variability is caused by axial rotation of a star with a variable degree of nonuniformity of the surface brightness (spots) and chromospheric activity. Some of these stars also show flares similar to those of UV Cet stars, and in those cases they also belong to the latter type and are simultaneously considered eruptive variables. |