The visual band light curve of ET Andromedae, adapted from Blanco et al. (1980) | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23 17 56.011185 |
Declination | +45° 29′ 20.1197″ |
Apparent magnitude (V) | 6.48 |
Characteristics | |
Spectral type | A0 Vp SiSr or B9p SI |
B−V color index | −0.037±0.006 |
Variable type | α CVn |
Astrometry | |
Radial velocity (Rv) | −0.30±4.10 km/s |
Proper motion (μ) | RA: +24.740 mas/yr Dec.: −11.038 mas/yr |
Parallax (π) | 5.4200 ± 0.0572 mas |
Distance | 602 ± 6 ly (185 ± 2 pc) |
Absolute magnitude (MV) | 0.58 |
Orbit | |
Period (P) | 48.304±0.007 d |
Eccentricity (e) | 0.50±0.05 |
Periastron epoch (T) | 2443720.11±0.64 JD |
Argument of periastron (ω) (secondary) | 49.8±6.0° |
Semi-amplitude (K1) (primary) | 25.7±2.0 km/s |
Details | |
Mass | 3.25 M☉ |
Radius | 2.7 R☉ |
Luminosity | 91.06 L☉ |
Surface gravity (log g) | 3.81 cgs |
Temperature | 11,444 K |
Rotation | 1.62 d |
Rotational velocity (v sin i) | 65 km/s |
Age | 284 Myr |
Other designations | |
AG+45° 2124, BD+44° 4373, HD 219749, HIP 115036, HR 8861, SAO 52876, PPM 64037, TYC 3636-2562-1, GSC 03636-02562, 2MASS J23175600+4529201 | |
Database references | |
SIMBAD | data |
ET Andromedae is a binary star system star in the northern constellation of Andromeda. It has an apparent visual magnitude of 6.48, placing it at the nominal limit for visibility with the naked eye. The distance to this system can be estimated from its annual parallax shift of 5.42 mas, which yields a value of 602 light years.
Variations in the radial velocity of this star suggest it is a single-lined spectroscopic binary system. This yields orbital elements with a period of 48.3 days and an eccentricity of 0.50. The a sin i value for the primary is 14.8 Gm (0.099 AU), where a is the semimajor axis and i is the (unknown) orbital inclination.
The visible component is a well-studied magnetic chemically peculiar star with a stellar classification of A0 Vp SiSr. The SiSr notation indicates unusual abundances of silicon and strontium in the spectrum. It has a magnetic field with an average surface value of 3.2 kT. The abundance of silicon varies depending on the viewing angle.
In 1953, Sanford S. Provin announced that HD 219749 might be photometrically variable, based on observations made at Yerkes Observatory. Variability was confirmed from Lowell Observatory measurements published by Karl D. Rakos in 1962. The star is an Alpha Canum Venaticorum variable with a period of 1.618875 days.
References
- Blanco, C.; Catalano, F. A.; Strazzulla, G. (January 1980). "The light variations of the Ap Star HR 8861". Astronomy & Astrophysics Supplement Series. 39: 127–128. Retrieved 8 October 2021.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
- ^ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ Abt, Helmut A.; Morrell, Nidia I. (1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". Astrophysical Journal Supplement. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182.
- Cowley, A.; et al. (April 1969). "A study of the bright A stars. I. A catalogue of spectral classifications". Astronomical Journal. 74: 375–406. Bibcode:1969AJ.....74..375C. doi:10.1086/110819.
- ^ Gontcharov, G. A. (November 2012). "Spatial distribution and kinematics of OB stars". Astronomy Letters. 38 (11): 694–706. arXiv:1606.09028. Bibcode:2012AstL...38..694G. doi:10.1134/S1063773712110035. S2CID 119108982.
- ^ Ouhrabka, M.; Grygar, J. (May 1979). "Spectroscopic evidence for the binary nature of the Ap star". Information Bulletin on Variable Stars. 1600: 1. Bibcode:1979IBVS.1600....1O.
- Ducati, J. R.; et al. (2011). "The mass ratio and initial mass functions in spectroscopic binaries" (PDF). Astronomy and Astrophysics. 525: A26. Bibcode:2011A&A...525A..26D. doi:10.1051/0004-6361/200913895. hdl:10183/99264.
- Pasinetti Fracassini, L. E.; et al. (2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy & Astrophysics. 367 (2) (Third ed.): 521–24. arXiv:astro-ph/0012289. Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID 425754.
- ^ Adelman, Saul J. (2002). "On the Periods of the Magnetic CP Stars". Baltic Astronomy. 11: 475–485. Bibcode:2002BaltA..11..475A.
- Kreidl, T. J. (October 1993), "A Null Detection of Rapid Oscillations in the Ap Star ET And", Information Bulletin on Variable Stars, 3945: 1, Bibcode:1993IBVS.3945....1K
- Strom, Stephen E.; et al. (2005). "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?". The Astronomical Journal. 129 (2): 809–828. arXiv:astro-ph/0410337. Bibcode:2005AJ....129..809S. doi:10.1086/426748. S2CID 15059129.
- "HD 13530". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 20 August 2018.
- Watson, Christopher (4 February 2010). "ET Andromedae". AAVSO Website. American Association of Variable Star Observers. Retrieved 5 November 2014.
- ^ Adelman, Saul J. (May 2000). "UVBY photometry of the magnetic CP stars HD 36668, 36 Lyncis, HD 86592, and HR 8861". Astronomy and Astrophysics. 357: 548–552. Bibcode:2000A&A...357..548A.
- Glagolevskij, Yu. V. (September 2007). "Magnetic-field dependence of chemical anomalies in CP stars". Astrophysical Bulletin. 62 (3): 244–256. Bibcode:2007AstBu..62..244G. doi:10.1134/S1990341307030054. S2CID 122706004.
- Provin, Sanford S. (November 1953). "Light-Variations of Peculiar a Stars". Astrophysical Journal. 118: 489–501. Bibcode:1953ApJ...118..489P. doi:10.1086/145777. Retrieved 30 October 2024.
- Rakos, Karl D. (1962). "Photoelectric investigation of magnetic and spectrum variable stars". Lowell Observatory Bulletin. 5 (117): 227. Bibcode:1962LowOB...5..227R. Retrieved 30 October 2024.
- Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017), "General catalogue of variable stars: Version GCVS 5.1", Astronomy Reports, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.
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