V0467 Persei
catalogues and names
| catalogues and names | V0467 Per, 42 Per, HR 1177, HD 23848, SAO 56727, BD +32 667 |
| constellation | Perseus |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
| position (J2000) | RA: 3h 49min 32.6sec | DEC: +33° 5' 29'' | ||
| position (B1900) | RA: 3h 43min 13.2sec | DEC: +32° 47' 5'' | ||
| proper motion (J2000) | RA: -0.029 arcsec/a | DEC: -0.001 arcsec/a | ||
| radial velocity | -14 km/s note: spectroscopic binaries note: orbital data avaible |
|||
| rotational velocity | 82 km/s (uncertain) (variable) | |||
| trigonometric parallax | -0.003 arcsec | |||
| galactic coordinates | longitude: 160.7° | latitude: -16.42° | ||
magnitude
| visual magnitude | 5.11 (V on UBV Johnson system) |
spectral / color information
| spectral class | A3V |
| B-V-magnitude | 0.07 |
| U-B-magnitude | 0.11 |
variability information
| variable star identification | V467 Per |
| note (category: variability): | A published period, 22.58d, does not satisfy available SB observations, whereas the SB period does satisfy the photometric equally well. However, more observations are badly needed. |
double/multiple star system information
| note (category: spectroscopic binaries): | 1.7653d, K 34.4k/s, V0 -11.9k/s, asini 0.832. |
miscellaneous information
| note (category: group membership): | Per OB2. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
| position (J2000) | RA: 3h 49min 32.685sec | DEC: +33° 5' 28.94'' | ±0.35 arcsec | source: 17 |
| proper motion (J2000) | RA: -0.0018 arcsec/a | DEC: 0.003 arcsec/a | source: 25 | |
| radial velocity | -14 km/s | source: 25 | ||
| galactic coord. (B1950) | longitude: 160.71° | latitude: -16.42° | ||
magnitude:
| visual | 5 (observed) | source: 31 |
| photovisual | 5.1 | source: 2 |
| photographic | 5.2 | source: 16 |
spectral information:
| spectral class | A2 | source: 96 | |
| Morgan-Keenan | A3V | source: 25 | |
| B-magnitude | 5.18 ±0.05 | B-V-magnitude | 0.07 |
| U-magnitude | 5.29 ±0.05 | U-B-magnitude | 0.11 |
variability information:
| variability type | 10 |
| var. amplitude | 0.13 |
| var. period | 22.58 |
| var. epoch | 2443101 18. November 1976, 12:00:00 UT |
| next max light | 2452223.32 9. November 2001, 19:40:48 UT |
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 | |
| 17 | ACRS |
| Corbin, T.E., and S.E. Urban, Astrographic Catalog Reference Stars, United States Naval Observatory, 1991 | |
| 25 | Bright Star Catalogue, 5th edition |
| Hoffleit, D. and Warren, W.H. Jr., The Bright Star Catalogue, 5th Revised Edition, Version 2, 1994 | |
| 30 | GCVS, 4th edition |
| Kholopov, P.N., et al., General Catalogue of Variable Stars, fourth edition, Moscow: Nauka Publishing House, 1985-88 | |
| 31 | CRM' (non-GCVS variable data) |
| 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: 3h 46min 22.612sec | DEC: +32° 56' 22.93'' | ±0.021 arcsec |
| position (J2000) | RA: 3h 49min 32.648sec | DEC: +33° 5' 28.8'' | |
| proper motion B1950 (FK4) | RA: -0.0023 arcsec/a | DEC: 0.001 arcsec/a | ±0.004 arcsec/a in RA ±0.003 arcsec/a in DEC |
| proper motion J2000 (FK5) | RA: -0.0023 arcsec/a | DEC: -0.001 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 | A2 |
| source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
| source catalogue | GC, catalogue number: 4592 |
| Durchmusterung | BD+32 667 |
| Boss General Catalogue | 4592 |
| Henry Draper Catalogue | 23848 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
| position (equinox 1950.0) | RA: 3h 46min 22.6sec | DEC: +32° 56' 23'' |
variability informations:
| variability type | E/D | close binary eclipsing system |
| magnitute at max. brightness | 5.05 | |
| magnitute at min. brightness | 5.18 | |
| photometric system | visual, photovisual or Johnson's V | |
| epoch for maximum light [JD] | 2443101.24 18. November 1976, 17:45:36 UT |
|
| period [d] | 22.58 | |
| next maximum light [JD] | 2452223.56 10. November 2001, 01:26:24 UT |
spectral information
| spectral class | A2V |
references
| to a study | Vol. I GCVS (see Kholopov et al. 1985-1988) |
| to a chart/photograph | no chart is avaible, but the star is contained in the 'Bonner Durchmusterung' |
miscanellous
| ID in the GCVS catalogue | 63/467 |
| constellation | Perseus |
| notes on existence | The star is equivalent to '0630468 V0468'. |
variability type description
| variability type | description |
| E | Eclipsing binary systems. These are binary systems with orbital planes so close to the observer's line of sight (the inclination i of the orbital plane to the plane orthogonal to the line of sight is close to 90 deg) that the components periodically eclipse each other. Consequently, the observer finds changes of the apparent combined brightness of the system with the period coincident with that of the components' orbital motion. EA Algol (Beta Persei)-type eclipsing systems. Binaries with spherical or slightly ellipsoidal components. It is possible to specify, for their light curves, the moments of the beginning and end of the eclipses. Between eclipses the light remains almost constant or varies insignificantly because of reflection effects, slight ellipsoidality of components, or physical variations. Secondary minima may be absent. An extremely wide range of periods is observed, from 0.2 to >= 10000 days. Light amplitudes are also quite different and may reach several magnitudes. EB Beta Lyrae-type eclipsing systems. These are eclipsing systems having ellipsoidal components and light curves for which it is impossible to specify the exact times of onset and end of eclipses because of a continuous change of a system's apparent combined brightness between eclipses; secondary minimum is observed in all cases, its depth usually being considerably smaller than that of the primary minimum; periods are mainly longer than 1 day. The components generally belong to early spectral types (B-A). Light amplitudes are usually <2 mag in V. EW W Ursae Majoris-type eclipsing variables. These are eclipsers with periods shorter than 1 days, consisting of ellipsoidal components almost in contact and having light curves for which it is impossible to specify the exact times of onset and end of eclipses. The depths of the primary and secondary minima are almost equal or differ insignificantly. Light amplitudes are usually <0.8 mag in V. The components generally belong to spectral types F-G and later. |
| D | Detached systems, with components not filling their inner Roche lobes. |