o Andromedae
catalogues and names
catalogues and names | o And, omi And, 1 And, HR 8762, HD 217675, SAO 52609, BD +41 4664, FK5: 869, WDS 23019+4220A |
constellation | Andromeda |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 23h 1min 55.3sec | DEC: +42° 19' 34'' | ||
position (B1900) | RA: 22h 57min 19.1sec | DEC: +41° 47' 19'' | ||
proper motion (J2000) | RA: 0.023 arcsec/a | DEC: -0.006 arcsec/a | ||
radial velocity | -14 km/s note: spectroscopic binaries, double lined spectra note: orbital data avaible |
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rotational velocity | 330 km/s (uncertain) (variable) | |||
trigonometric parallax | 0.015 arcsec | |||
galactic coordinates | longitude: 102.21° | latitude: -16.1° |
note (category: radial and/or rotational velocities): | 23.5y. vsini about 300k/s. |
magnitude
visual magnitude | 3.62 (V on UBV Johnson system) |
spectral / color information
spectral class | B6IIIpe+A2p |
B-V-magnitude | -0.09 |
U-B-magnitude | -0.53 |
R-I-magnitude |
note (category: spectra): | Shell star. Also classified B5III or B6IVpe. |
variability information
variable star identification | Omi And |
note (category: variability): | Gamma Cas 3.58 - 3.65V. Photometric investigations have indicated numerous periods, particularly 0.78823, 1.0815d and 1.5998398d, all doubtful. Form of light curve varies. Probably not an eclipsing binary. Period shell phenomena about 23.5y. Shell features have vanished several times since 1897. H gamma varies in 3.66?d. |
double/multiple star system information
number of components of multiple star system | 4 |
separation | 0.3 arcsec |
mag difference (of double or brightest multiple) | 0.5 |
component ID | S |
note | doublicity discoverd by speckle interferometry |
note (category: double and multiple data): | Separate speckle interferometric measures give sep. 0.05" (Aa) and 0.34" (AB). Ten years of observations reveal steady change in AB position angle of about 10d with decrease in separation from about 0.375" to 0.266". Component B identified as SB2 (see SB remarks), making total number of components at least 4. |
note (category: spectroscopic binaries): | Speckle interferometry indicates triple star. SB periods 72.3145, 8585 or 9478d. Also short period 1.5845, 0.84, 3.66 or 1.67458d, all doubtful. Observations by Hill et al. (1988, PASP, 100, 243) indicate that one of the companions of A is SB2, and they identify this as component B. Orbit for B: 33.01d, V0 -14.3k/s, K1 54.8k/s, K2 71.6k/s, m1sin3i 3.74, m2sin3i 2.86, a1sini 0.161, a2sini 0.211. |
miscellaneous information
note (category: group membership): | In reflection nebula; probably but not certainly associated. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 23h 1min 55.267sec | DEC: +42° 19' 33.5'' | ±0.06 arcsec | source: 15 |
proper motion (J2000) | RA: 0.002 arcsec/a | DEC: -0.006 arcsec/a | source: 25 | |
radial velocity | -14 km/s | source: 25 | ||
trigonometric parallax | 0.015 arcsec | ±0.002 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 102.21° | latitude: -16.1° |
magnitude:
visual | 3.62 (observed) | source: 25 |
photovisual | 3.6 | source: 2 |
spectral information:
spectral class | B5 | source: 96 | |
Morgan-Keenan | B6IIIpe | source: 25 | |
B-magnitude | 3.53 ±0.05 | B-V-magnitude | -0.09 |
U-magnitude | 3 ±0.05 | U-B-magnitude | -0.53 |
variability information:
variability type | 264 |
var. amplitude | 0.2 |
double/multiple star system information:
separation between brightest and second brightest component | 0.1 arcsec |
component | magnitude | spectral class | catalogue(s)/name(s) |
A | 3.62 | B5 | o Andromedae, 1 And, HR 8762, HD 217675, SAO 52609 |
B | 3.58 | +++ |
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 | |
15 | FK5, FK5 Extension and FK5 Supplement |
Fricke, W., H. Schwan and T. Lederle, "Fifth Fundamental Catalogue (FK5), Part I. The Basic Fundamental Stars," Veroff. Astronomisches Recheninstitut, No. 32, Heidelberg, Germany, 1988, and Fricke, W., H. Schwan, and T.E. Corbin, "Fifth Fundamental Catalogue (FK5), Part II. The FK5 Extension," Veröff. Astronomisches Recheninstitut, No. 33, Heidelberg, Germany, 1991 | |
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: 22h 59min 36.873sec | DEC: +42° 3' 25.12'' | ±0.004 arcsec |
position (J2000) | RA: 23h 1min 55.27sec | DEC: +42° 19' 33.65'' | |
proper motion B1950 (FK4) | RA: 0.0019 arcsec/a | DEC: 0 arcsec/a | ±0.001 arcsec/a in RA ±0.001 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: 0.0021 arcsec/a | DEC: -0.005 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 3.6 (accuracy: 2 decimals) |
source of visual magnitude data | Arithmetic mean of maximum and minimum magnitudes of a variable star |
spectral information:
spectral class | +++ |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
remarks for duplicity and variability
Variable star in visual magnitude in source catalog |
catalogues
source catalogue | FK4, catalogue number: 869 |
Durchmusterung | BD+41 4664 |
Boss General Catalogue | 32095 |
Henry Draper Catalogue | 217675 The "SAO Catalog" entry refers to two consecutive HD numbers, the lower of which is given. |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 23h 1.9min | DEC: +42° 20' |
proper motion (J2000) | RA: 0.023 arcsec/a | DEC: -0.006 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 |
Aa | 1975 | 8 | ° | 0.1'' | 3.62 | - | B6III+A2 | BLA |
Aa-B | 1976 | 37 | 7° | 0.4'' | 3.6 | - | - | WRH |
1993 | 340° | 0.2'' |
discoverer information:
discoverer code | discoverer | reference |
BLA | Blazit, A. et al | |
WRH | Wilson, R.H. |
notes:
note | Aa: Omicron And. Spectrum composite: B6IIIpe+A2p. There appear to be both short and long period light variations. Aa-B: P = 68.6yr., a = 0.277", motion retrograde. B has been reported to be a double-lined spectroscopic binary, P = 33.01d. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 22h 59min 36.9sec | DEC: +42° 3' 25'' |
variability informations:
variability type | GCAS | eruptive variable star |
magnitute at max. brightness | 3.58 | |
magnitute at min. brightness | 3.78 | |
photometric system | visual, photovisual or Johnson's V |
spectral information
spectral class | B6IIIpe+A2p |
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 | 1/9015 |
constellation | Andromeda |
There are notes in published catalog. |
variability type description
variability type | description |
GCAS | Eruptive irregular variables of the Gamma Cas type. These are rapidly rotating B III-IVe stars with mass outflow from their equatorial zones. The formation of equatorial rings or disks is often accompanied by temporary fading. Light amplitudes may reach 1.5 mag in V. |