V0535 Arae
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 | V0535 Ara, HD 159441, SAO 244895, CP -56 8348 |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 17h 38min 5.532sec | DEC: -56° 49' 17.2'' | ±0.18 arcsec | source: 16 |
position (2000.73) | RA: 17h 38min 10sec | DEC: -56° 49' 18'' | JD: 2451810.12 | |
proper motion (J2000) | RA: -0.0097 arcsec/a | DEC: -0.047 arcsec/a | source: 16 | |
galactic coord. (B1950) | longitude: 335.18° | latitude: -13.2° |
magnitude:
visual | 7.17 (observed) | source: 30 |
photovisual | 7.7 | source: 16 |
spectral information:
spectral class | A3 | source: 96 | |
Morgan-Keenan | A8V | source: 10 |
variability information:
variability type | 10 |
var. amplitude | 0.58 |
var. period | 0.63 |
var. epoch | 2439293 16. June 1966, 12:00:00 UT |
next max light | 2451810.47 22. September 2000, 23:16:48 UT |
sources:
10 | Michigan Catalog of 2-Dimensional Spectral Types for the HD Stars, Volumes I-III |
Houk, N., and A.P. Cowley, Michigan Catalogue of 2-Dimensional Spectral Types for the HD Stars, Vol. 1., (Zones -89 to -53 Degrees), Ann Arbor: The University of Michigan, 1975, and Houk, N., Michigan Catalogue of 2-Dimensional Spectral Types for the HD Stars, Vol. 2., (Zones -52 to -40 Degrees), Ann Arbor: The University of Michigan, 1978, and Houk, N., Michigan Catalogue of 2-Dimensional Spectral Types for the HD Stars, Vol. 3., (Zones -40 to -26 Degrees), Ann Arbor: The University of Michigan, 1982 | |
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 | |
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: 17h 33min 50.722sec | DEC: -56° 47' 28.93'' | ±0.058 arcsec |
position (2000.73) | RA: 17h 38min 10sec | DEC: -56° 49' 15'' | JD: 2451810.12 |
position (J2000) | RA: 17h 38min 5.709sec | DEC: -56° 49' 15.63'' | |
proper motion B1950 (FK4) | RA: -0.007 arcsec/a | DEC: -0.033 arcsec/a | ±0.012 arcsec/a in RA ±0.009 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.0076 arcsec/a | DEC: -0.035 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 7.5 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | A3 |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | GC, catalogue number: 23860 |
Durchmusterung | CP-56 8348 |
Boss General Catalogue | 23860 |
Henry Draper Catalogue | 159441 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 17h 33min 50.7sec | DEC: -56° 47' 29'' |
variability informations:
variability type | EW/DW: | close binary eclipsing system |
magnitute at max. brightness | 7.17 | |
magnitute at min. brightness | 7.75 | |
photometric system | visual, photovisual or Johnson's V | |
epoch for maximum light [JD] | 2439292.9353 16. June 1966, 10:26:50 UT |
|
period [d] | 0.62929677 | |
next maximum light [JD] | 2451810.27735207 22. September 2000, 18:39:23 UT |
spectral information
spectral class | A8V |
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 | 6/535 |
constellation | Ara |
notes on existence | The star is equivalent to '0060536 V0536'. |
There are notes in published catalog. |
variability type description
variability type | description |
EW | 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. |
DW | Systems similar to W UMa systems in physical properties (KW, see below), but not in contact. |