R Trianguli Australis
catalogues and names |
SKY2000 - Master Star Catalog |
Smithsonian Astrophysical Observatory Star Catalog |
Combined General Catalogue of Variable Stars (Vol. I-III) |
catalogues and names
catalogues and names | R TrA, HD 135592, SAO 253107, CP -66 2753 |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 15h 19min 45.711sec | DEC: -66° 29' 45.7'' | ±0.19 arcsec | source: 16 |
position (2000.72) | RA: 15h 19min 50sec | DEC: -66° 29' 55'' | JD: 2451806.24 | |
proper motion (J2000) | RA: -0.0008 arcsec/a | DEC: -0.008 arcsec/a | source: 16 | |
radial velocity | -14 km/s | source: 26 | ||
galactic coord. (B1950) | longitude: 316.98° | latitude: -7.76° |
magnitude:
visual | 6.33 (observed) | source: 30 |
photovisual | 6.7 | source: 16 |
spectral information:
spectral class | F5 | source: 96 | |
Morgan-Keenan | F7Ib/II | source: 26 | |
B-magnitude | 6.96 ±0.2 | B-V-magnitude | 0.57 |
U-magnitude | 7.29 ±0.2 | U-B-magnitude | 0.33 |
variability information:
variability type | 111 |
var. amplitude | 0.67 |
var. period | 3.39 |
var. epoch | 2440838 8. September 1970, 12:00:00 UT |
next max light | 2451808.04 20. September 2000, 12:57:36 UT |
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 | |
26 | Bright Star Supplement |
Hoffleit, D. and Warren, W.H. Jr., A Supplement to the Bright Star Catalogue, 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: 15h 15min 15.872sec | DEC: -66° 18' 53.37'' | ±0.057 arcsec |
position (2000.72) | RA: 15h 19min 50sec | DEC: -66° 29' 55'' | JD: 2451806.24 |
position (J2000) | RA: 15h 19min 45.663sec | DEC: -66° 29' 46.95'' | |
proper motion B1950 (FK4) | RA: -0.0003 arcsec/a | DEC: -0.022 arcsec/a | ±0.011 arcsec/a in RA ±0.01 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.0017 arcsec/a | DEC: -0.017 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
photographic | 7.1 (accuracy: 1 decimal) |
source of photographic magnitude data | Source cited in source catalog introduction. |
spectral information:
spectral class | G0v |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
remarks for duplicity and variability
Variable star in photographic magnitude in source catalog |
catalogues
source catalogue | GC, catalogue number: 20561 |
Durchmusterung | CP-66 2753 |
Boss General Catalogue | 20561 |
Henry Draper Catalogue | 135592 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 15h 15min 15.9sec | DEC: -66° 18' 53'' |
variability informations:
variability type | DCEP | pulsating variable star |
magnitute at max. brightness | 6.33 | |
magnitute at min. brightness | 7 | |
photometric system | visual, photovisual or Johnson's V | |
epoch for maximum light [JD] | 2440838.21 8. September 1970, 17:02:24 UT |
|
period [d] | 3.389287 | |
next maximum light [JD] | 2451809.332019 21. September 2000, 19:58:06 UT |
|
rising time | 30 % of period |
spectral information
spectral class | F6Ib/II-G0 |
references
to a study | Vol. I GCVS (see Kholopov et al. 1985-1988) |
to a chart/photograph | Vol. I GCVS (see Kholopov et al. 1985-1988) |
miscanellous
ID in the GCVS catalogue | 81/1 |
constellation | Triangulum Australe |
notes on existence | The star is equivalent to '0810002 S'. |
There are notes in published catalog. |
variability type description
variability type | description |
DCEP | These are the classical cepheids, or Delta Cep-type variables. Comparatively young objects that have left the main sequence and evolved into the instability strip of the Hertzsprung-Russell (H-R) diagram, they obey the well-known Cepheid period-luminosity relation and belong to the young disk population. DCEP stars are present in open clusters. They display a certain relation between the shapes of their light curves and their periods. |