V4200 Sagittarii
catalogues and names
catalogues and names | V4200 Sgr, HR 7578, HD 188088, SAO 188692, CD -24 15668, WDS 19543-2356 |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 19h 54min 17.7sec | DEC: -23° 56' 28'' | ||
position (2000.72) | RA: 19h 54min 21sec | DEC: -23° 56' 21'' | ||
position (B1900) | RA: 19h 48min 18.4sec | DEC: -24° 11' 23'' | ||
proper motion (J2000) | RA: -0.131 arcsec/a | DEC: -0.414 arcsec/a | ||
radial velocity | -7 km/s note: spectroscopic binaries, double lined spectra |
|||
rotational velocity | =<8 km/s (uncertain) (variable) | |||
trigonometric parallax | 0.075 arcsec | |||
galactic coordinates | longitude: 17.18° | latitude: -23.91° |
magnitude
visual magnitude | 6.18 (V on UBV Johnson system) |
spectral / color information
spectral class | K2V |
B-V-magnitude | 1.02 |
U-B-magnitude | 0.94 |
R-I-magnitude |
variability information
variable star identification | Var? |
note (category: variability): | BY Dra type predicted, but variability not yet detected. |
double/multiple star system information
separation | 31.5 arcsec |
mag difference (of double or brightest multiple) | 4 |
note (category: double and multiple data): | Optical. |
note (category: spectroscopic binaries): | 46.817d, e 0.692, K(A) 48.8 k/s, K(B) 48.7 k/s, V0 -5.1 k/s, m(A)sin3i = m(B)sin3i = 0.85, a(A)sini 22.7, a(B)sini 22.6. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 19h 54min 17.755sec | DEC: -23° 56' 27.82'' | ±0.19 arcsec | source: 16 |
position (2000.72) | RA: 19h 54min 21sec | DEC: -23° 56' 21'' | JD: 2451809.16 | |
proper motion (J2000) | RA: -0.0088 arcsec/a | DEC: -0.409 arcsec/a | source: 25 | |
radial velocity | -7 km/s | source: 25 | ||
trigonometric parallax | 0.075 arcsec | ±0.007 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 17.19° | latitude: -23.91° |
magnitude:
visual | 6.18 (observed) | source: 25 |
photovisual | 6.1 | source: 16 |
spectral information:
spectral class | K0 | source: 96 | |
Morgan-Keenan | K3VaCN1 | source: 25 | |
B-magnitude | 7.2 ±0.05 | B-V-magnitude | 1.02 |
U-magnitude | 8.14 ±0.05 | U-B-magnitude | 0.94 |
double/multiple star system information:
separation between brightest and second brightest component | 31.5 arcsec |
magnitude difference between brightest and second brightest component | 4.1 |
position angle | 46 ° |
sources:
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 | |
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: 19h 51min 18.168sec | DEC: -24° 4' 1.24'' | ±0.018 arcsec |
position (2000.72) | RA: 19h 54min 21sec | DEC: -23° 56' 1'' | JD: 2451809.16 |
position (J2000) | RA: 19h 54min 17.692sec | DEC: -23° 56' 28.26'' | |
proper motion B1950 (FK4) | RA: -0.0097 arcsec/a | DEC: -0.412 arcsec/a | ±0.004 arcsec/a in RA ±0.004 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.0096 arcsec/a | DEC: -0.414 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 6.3 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | K0 |
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: 27542 |
Durchmusterung | CD-2415668 |
Boss General Catalogue | 27542 |
Henry Draper Catalogue | 188088 |
data from The Washington Visual Double Star Catalog, 1996.0 (Worley+, 1996)
position and proper motion:
position (J2000) | RA: 19h 54.3min | DEC: -23° 56' |
proper motion (J2000) | RA: -0.121 arcsec/a | DEC: -0.409 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 |
- | 1877 | 18 | 142° | 18.3'' | 6.18 | 10.3 | K3IV | HJ 2904 |
1965 | 46° | 31.5'' |
discoverer information:
discoverer code | discoverer | reference |
HJ 2904 | Herschel, J. | - |
notes:
note | A is a spectroscopic binary. |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 19h 51min 18.2sec | DEC: -24° 4' 1'' |
variability informations:
variability type | BY | rotating variable star |
magnitute at max. brightness | 6.18 | |
magnitute amplitude | 0.07 | |
photometric system | visual, photovisual or Johnson's V |
references
to a study | J.T.Hooten, D.S.Hall, ApJ Suppl 74, No.1, 225, 1990. |
to a chart/photograph | no chart is avaible, but the star is contained in the 'Cordoba Durchmusterung' |
miscanellous
ID in the GCVS catalogue | 72/4200 |
constellation | Sagittarius |
notes on existence | The star is equivalent to '71399'. |
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. |