l Tauri
| catalogues and names | l Tau, lam Tau, 35 Tau, HR 1239, HD 25204, SAO 93719, FK5: 150 |
| constellation | Taurus |
data from The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) (Hoffleit+, 1991)
position, motion, parallax:
| position (J2000) | RA: 4h 0min 40,8sec | DEC: +12° 29' 25'' |
| position (J1900) | RA: 3h 55min 8,3sec | DEC: +12° 12' 28'' |
| proper motion (J2000) | RA: -0,006 arcsec/a | DEC: -0,012 arcsec/a |
| radial velocity | 18 km/s note: spectroscopic binaries, double lined spectra note: orbital data avaible |
|
| rotational velocity | 87 km/s (uncertain) (variable) | |
| trigonometric parallax | 0,002 arcsec | |
| note (category: dynamical parallaxes): | 0.0042". |
magnitude
| visual magnitude | 3,47 (V on UBV Johnson system) |
spectral / color information
| spectral class | B3V+A4IV |
| B-V-magnitude | -0,12 |
| U-B-magnitude | -0,62 |
| R-I-magnitude | -0,09 |
variability information
| variable star identification | Lam Tau |
| note (category: variability): | EA 3.3 - 3.80p, B3V+A, 3.952955d, i 86d. |
double/multiple star system information
| note (category: spectroscopic binaries): | 3.9540d, K 55.4k/s, V0 +15.2k/s, asini 2.99. RV also varies in 33.025d, triple system. Masses 6.8, 1.8 and about 1 solar. |
data from SKY2000 - Master Star Catalog (Myers+ 1997)
position, motion, parallax:
| position (J2000) | RA: 4h 0min 40,819sec | DEC: +12° 29' 25,24'' | ±0,06 arcsec | source: 15 |
| proper motion (J2000) | RA: -0,0004 arcsec/a | DEC: -0,012 arcsec/a | source: 25 | |
| radial velocity | 18 km/s | source: 25 | ||
| trigonometric parallax | 0,002 | - | source: 25 | |
| galactic coord. (B1950) | longitude: 178,38° | latitude: -29,38° | ||
| GCI unit vector (J2000) | X: 0,485654 | Y: 0,846974 | Z: 0,216275 | |
magnitude:
| visual | 3,4 (observed) | source: 31 |
spectral information:
| spectral class | B3 | source: 96 | |
| Morgan-Keenan | B3V+A4IV | source: 25 | |
| B-magnitude | 3,35 ±0,05 | B-V-magnitude | -0,12 |
| U-magnitude | 2,73 ±0,05 | U-B-magnitude | -0,62 |
variability information:
| variability type | 10 |
| var. amplitude | 0,54 |
| var. period | 3,95 |
| var. epoch | 2421507 5. October 1917, 12:00:00 UT |
| next max light | 2451625,75 22. March 2000, 06:00:00 UT |
sources:
| 15 | FK5, FK5 Extension and FK5 Supplement |
| Fricke, W., H. Schwan and T. Lederle, "Fifth Fundamental Catalogue (FK5), Part I. The Basic Fundamental Stars," Veroff. Astronomisches Recheninstitut, No. 32, Heidelberg, Germany, 1988, and Fricke, W., H. Schwan, and T.E. Corbin, "Fifth Fundamental Catalogue (FK5), Part II. The FK5 Extension," Veröff. Astronomisches Recheninstitut, No. 33, Heidelberg, Germany, 1991 | |
| 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 | |
| 31 | CRM' (non-GCVS variable data) |
| Warren, W.H. Jr., Northern Hemisphere Catalog of Red Magnitudes, 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 (J1950) | RA: 3h 57min 54,378sec | DEC: +12° 21' 2,13'' | ±0,004 arcsec |
| position (J2000) | RA: 4h 0min 40,822sec | DEC: +12° 29' 25,33'' | |
| proper motion J1950 (FK4) | RA: -0,0005 arcsec/a | DEC: -0,009 arcsec/a | ±0,001 arcsec/a in RA ±0,001 arcsec/a in DEC |
| proper motion J2000 (FK5) | RA: -0,0004 arcsec/a | DEC: -0,011 arcsec/a | |
| source of proper motion data | Determined by source catalog | ||
magnitude:
| visual | 4 (accuracy: 2 decimals) |
| source of visual magnitude data | Arithmetic mean of maximum and minimum magnitudes of a variable star |
spectral information:
| spectral class | B3 |
| source of spectral data | Taken from the Henry Draper Catalogue or no spectrum in source catalog. |
remarks for duplicity and variability
| Variable star in visual magnitude in source catalog |
catalogues
| source catalogue | FK4, catalogue number: 150 |
| Durchmusterung | BD+12 539 |
| Boss General Catalogue | 4805 |
| Henry Draper Catalogue | 25204 |
data from Combined General Catalogue of Variable Stars (Vol. I-III) (Kholopov+ 1998)
position:
| position (J1950) | RA: 3h 57min 54,4sec | DEC: +12° 21' 2'' |
variability informations:
| variability type | EA/DM | close binary eclipsing system |
| magnitute at max. brightness | 3,37 | |
| magnitute at min. brightness | 3,91 | |
| photometric system | visual, photovisual or Johnson's V | |
| epoch for maximum light [JD] | 2421506,8506 5. October 1917, 08:24:52 UT |
|
| period [d] | 3,9529478 | |
| next maximum light [JD] | 2451624,3598882 20. March 2000, 20:38:14 UT |
|
| duration of the eclipse | 15 % of period the duration of the light constancy phase at minimum light is equal to zero |
spectral information
| spectral class | B3V+A4IV |
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 | 78/9011 |
| constellation | Taurus |
| notes on existence | The star is equivalent to '0789017 rho'. |
| There are notes in published catalog. | |
variability type description
| variability type | description |
| EA | 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. |
| DM | Detached main-sequence systems. Both components are main-sequence stars and do not fill their inner Roche lobes. |