AX Microscopii
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 | AX Mic, HD 202560, SAO 212866, CD -39 14192 |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
position (J2000) | RA: 21h 17min 15.185sec | DEC: -38° 52' 3.06'' | ±0.19 arcsec | source: 16 |
position (2000.73) | RA: 21h 17min 18sec | DEC: -38° 51' 53'' | JD: 2451812.24 | |
proper motion (J2000) | RA: -0.28 arcsec/a | DEC: -1.153 arcsec/a | source: 16 | |
radial velocity | 20 km/s | source: 26 | ||
trigonometric parallax | 0.261 arcsec | ±0.026 arcsec | source: 26 | |
galactic coord. (B1950) | longitude: 3.93° | latitude: -44.3° |
magnitude:
visual | 6.68 (observed) | source: 26 |
photovisual | 6.7 | source: 2 |
spectral information:
spectral class | M0 | source: 96 | |
Morgan-Keenan | M0Ve | source: 26 | |
B-magnitude | 8.09 ±0.2 | B-V-magnitude | 1.41 |
U-magnitude | 9.3 ±0.2 | U-B-magnitude | 1.21 |
variability information:
variability type | 220 |
var. amplitude | 0.1 |
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 | |
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: 21h 14min 19.947sec | DEC: -39° 3' 42.45'' | ±0.065 arcsec |
position (2000.73) | RA: 21h 17min 32sec | DEC: -38° 50' 55'' | JD: 2451812.24 |
position (J2000) | RA: 21h 17min 15.232sec | DEC: -38° 52' 4.5'' | |
proper motion B1950 (FK4) | RA: -0.2805 arcsec/a | DEC: -1.152 arcsec/a | ±0.011 arcsec/a in RA ±0.011 arcsec/a in DEC |
proper motion J2000 (FK5) | RA: -0.2793 arcsec/a | DEC: -1.166 arcsec/a | |
source of proper motion data | Determined by source catalog |
magnitude:
visual | 6.6 (accuracy: 2 decimals) |
source of visual magnitude data | Taken from Harvard or San Luis photometry. |
spectral information:
spectral class | M0p |
source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
catalogues
source catalogue | GC, catalogue number: 29761 |
Durchmusterung | CD-3914192 |
Boss General Catalogue | 29761 |
Henry Draper Catalogue | 202560 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
position (equinox 1950.0) | RA: 21h 14min 19.9sec | DEC: -39° 3' 42'' |
variability informations:
variability type | UV | eruptive variable star |
magnitute at max. brightness | 9.21 | |
magnitute at min. brightness | 9.31 | |
photometric system |
spectral information
spectral class | M0Ve |
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 'Cordoba Durchmusterung' |
miscanellous
ID in the GCVS catalogue | 54/77 |
constellation | Microscopium |
notes on existence | The star is equivalent to '0540078 AY'. |
There are notes in published catalog. |
variability type description
variability type | description |
UV | Eruptive variables of the UV Ceti type, these are K Ve-M Ve stars sometimes displaying flare activity with amplitudes from several tenths of a magnitude up to 6 mag in V. The amplitude is considerably greater in the ultraviolet spectral region. Maximum light is attained in several seconds or dozens of seconds after the beginning of a flare; the star returns to its normal brightness in several minutes or dozens of minutes. |