V0474 Persei
catalogues and names
catalogues and names | V0474 Per, 9 Per, HR 685, HD 14489, SAO 23256, BD +55 598, FK5: 2159, WDS 02224+5551 |
constellation | Perseus |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 2h 22min 21.4sec | DEC: +55° 50' 44'' | ||
position (B1900) | RA: 2h 15min 22.8sec | DEC: +55° 23' 17'' | ||
proper motion (J2000) | RA: -0.002 arcsec/a | DEC: -0.002 arcsec/a | ||
radial velocity | -15 km/s note: variable radial velocity |
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rotational velocity | 25 km/s (uncertain) (variable) | |||
galactic coordinates | longitude: 135.51° | latitude: -4.79° |
note (category: radial and/or rotational velocities): | Var. in period over 200d. |
magnitude
visual magnitude | 5.17 (V on UBV Johnson system) |
spectral / color information
spectral class | A2Ia |
B-V-magnitude | 0.37 |
U-B-magnitude | -0.11 |
R-I-magnitude |
note (category: spectra): | Shell star. |
variability information
variable star identification | V474 Per |
note (category: variability): | Amp. 0.05V. Sp. and H alpha profile var. |
double/multiple star system information
separation | 11.6 arcsec |
mag difference (of double or brightest multiple) | 7.8 |
note (category: double and multiple data): | Fixed. |
miscellaneous information
note (category: group membership): | Per OB1. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 2h 22min 21.429sec | DEC: +55° 50' 45.44'' | ±0.43 arcsec | source: 16 |
proper motion (J2000) | RA: -0.0001 arcsec/a | DEC: 0.017 arcsec/a | source: 25 | |
radial velocity | -15 km/s | source: 25 | ||
galactic coord. (B1950) | longitude: 135.51° | latitude: -4.79° |
magnitude:
visual | 5.17 (observed) | source: 25 |
photovisual | 5.2 | source: 2 |
photographic | 5.3 | source: 16 |
spectral information:
spectral class | A2 | source: 96 | |
Morgan-Keenan | A2Ia | source: 25 | |
B-magnitude | 5.54 ±0.05 | B-V-magnitude | 0.37 |
U-magnitude | 5.43 ±0.05 | U-B-magnitude | -0.11 |
variability information:
variability type | 133 |
var. amplitude | 0.1 |
double/multiple star system information:
separation between brightest and second brightest component | 11.6 arcsec |
magnitude difference between brightest and second brightest component | 6 |
position angle | 162 ° |
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 | |
27 | Catalog of Red Magnitudes (CRM) |
Warren, W.H. Jr., Northern Hemisphere Catalog of Red Magnitudes, 1994 | |
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: 2h 18min 51.207sec | DEC: +55° 37' 5.42'' | ±0.018 arcsec |
position (J2000) | RA: 2h 22min 21.4sec | DEC: +55° 50' 44.63'' | |
proper motion B1950 (FK4) | RA: -0.0001 arcsec/a | DEC: 0.004 arcsec/a | ±0.003 arcsec/a in RA ±0.002 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.0002 arcsec/a | DEC: 0 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 5.2 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | A2p |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
remarks for duplicity and variability
Double star in Aitken's Double Star Catalogue (Aitken 1932) |
catalogues
source catalogue | GC, catalogue number: 2836 |
Durchmusterung | BD+55 598 |
Boss General Catalogue | 2836 |
Henry Draper Catalogue | 14489 |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 2h 22.4min | DEC: +55° 51' |
proper motion (J2000) | RA: -0.003 arcsec/a | DEC: -0.004 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 |
- | 1880 | 8 | 162° | 11.6'' | 6 | 12 | A2Ia | BU 875 |
discoverer information:
discoverer code | discoverer | reference |
BU 875 | Burnham, S.W. | - |
notes:
note | 9 Per. Variable, V474 Per. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 2h 18min 51.2sec | DEC: +55° 37' 5'' |
variability informations:
variability type | ACYG | pulsating variable star |
magnitute at max. brightness | 5.15 | |
magnitute at min. brightness | 5.25 | |
photometric system | visual, photovisual or Johnson's V |
references
to a study | F.Rufener, A.Maeder, G.Burki, AsAp Suppl 31,179,1978. |
to a chart/photograph | no chart is avaible, but the star is contained in the 'Bonner Durchmusterung' |
miscanellous
ID in the GCVS catalogue | 63/474 |
constellation | Perseus |
notes on existence | The star is equivalent to '67039'. |
variability type description
variability type | description |
ACYG | Variables of the Alpha Cygni type, which are nonradially pulsating supergiants of Bep-AepIa spectral types. The light changes with amplitudes of the order of 0.1 mag often seem irregular, being caused by the superposition of many oscillations with close periods. Cycles from several days to several weeks are observed. |