r1Sagittarii
catalogues and names
catalogues and names | r1Sgr, rho 1 Sgr, 44 Sgr, HR 7340, HD 181577, SAO 162512, BD -18 5322 |
constellation | Sagittarius |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
position (J2000) | RA: 19h 21min 40.4sec | DEC: -17° 50' 50'' | ||
position (2000.73) | RA: 19h 21min 43sec | DEC: -17° 50' 45'' | ||
position (B1900) | RA: 19h 15min 52.4sec | DEC: -18° 2' 8'' | ||
proper motion (J2000) | RA: -0.024 arcsec/a | DEC: 0.024 arcsec/a | ||
radial velocity | 1 km/s | |||
rotational velocity | 68 km/s (uncertain) (variable) | |||
trigonometric parallax | 0.042 arcsec | |||
galactic coordinates | longitude: 20.06° | latitude: -14.55° |
magnitude
visual magnitude | 3.93 (V on UBV Johnson system) |
spectral / color information
spectral class | F0IV-V |
B-V-magnitude | 0.22 |
U-B-magnitude | 0.13 |
R-I-magnitude |
variability information
variable star identification | Rho1 Sgr |
note (category: variability): | Delta Sct 3.90 - 3.93V, 0.050d. |
double/multiple star system information
separation | 0 arcsec |
mag difference (of double or brightest multiple) | 2.5 |
note | doublicity discoverd by occultation |
note (category: double and multiple data): | Sep. 0.036". Questionable occultation double. |
miscellaneous information
note (category: group membership): | Possible Eggen group with HR 63, q.v. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 19h 21min 40.345sec | DEC: -17° 50' 50.3'' | ±0.19 arcsec | source: 16 |
position (2000.73) | RA: 19h 21min 43sec | DEC: -17° 50' 45'' | JD: 2451810.88 | |
proper motion (J2000) | RA: -0.0018 arcsec/a | DEC: 0.018 arcsec/a | source: 25 | |
radial velocity | 1 km/s | source: 25 | ||
trigonometric parallax | 0.042 arcsec | ±0.004 arcsec | source: 25 | |
galactic coord. (B1950) | longitude: 20.06° | latitude: -14.55° |
magnitude:
visual | 3.93 (observed) | source: 25 |
photovisual | 4 | source: 2 |
photographic | 4.1 | source: 2 |
spectral information:
spectral class | A5 | source: 96 | |
Morgan-Keenan | F0IV-V | source: 25 | |
B-magnitude | 4.15 ±0.05 | B-V-magnitude | 0.22 |
U-magnitude | 4.28 ±0.05 | U-B-magnitude | 0.13 |
variability information:
variability type | 10 |
var. amplitude | 0.04 |
var. period | 0.05 |
double/multiple star system information:
separation between brightest and second brightest component | 0 arcsec |
magnitude difference between brightest and second brightest component | 2.5 |
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 | |
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 | |
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 18min 46.401sec | DEC: -17° 56' 34.67'' | ±0.015 arcsec |
position (2000.73) | RA: 19h 21min 43sec | DEC: -17° 50' 46'' | JD: 2451810.88 |
position (J2000) | RA: 19h 21min 40.371sec | DEC: -17° 50' 49.73'' | |
proper motion B1950 (FK4) | RA: -0.0018 arcsec/a | DEC: 0.024 arcsec/a | ±0.002 arcsec/a in RA ±0.002 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.0017 arcsec/a | DEC: 0.024 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 4 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | A5 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | GC, catalogue number: 26694 |
Durchmusterung | BD-18 5322 |
Boss General Catalogue | 26694 |
Henry Draper Catalogue | 181577 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 19h 18min 46.4sec | DEC: -17° 56' 35'' |
variability informations:
variability type | DSCTC | pulsating variable star |
magnitute at max. brightness | 3.9 | |
magnitute at min. brightness | 3.94 | |
photometric system | visual, photovisual or Johnson's V | |
period [d] | 0.05 |
spectral information
spectral class | F0IV-V |
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 | 72/90171 |
constellation | Sagittarius |
notes on existence | The star is equivalent to '0729020 ups'. |
variability type description
variability type | description |
DSCTC | Variables of the Delta Scuti type. These are pulsating variables of spectral types A0-F5 III-V displaying light amplitudes from 0.003 to 0.9 mag in V (usually several hundredths of a magnitude) and periods from 0.01 to 0.2 days. The shapes of the light curves, periods, and amplitudes usually vary greatly. Radial as well as nonradial pulsations are observed. The variability of some members of this type appears sporadically and sometimes completely ceases, this being a consequence of strong amplitude modulation with the lower value of the amplitude not exceeding 0.001 mag in some cases. The maximum of the surface layer expansion does not lag behind the maximum light for more than 0.1 periods. DSCT stars are representatives of the galactic disk (flat component) and are phenomenologically close to the SX Phe variables. DSCTC Low amplitude group of Delta Sct variables (light amplitude <0.1 mag in V). The majority of this type's representatives are stars of luminosity class V; objects of this subtype generally are representative of the Delta Sct variables in open clusters. |