Misplaced Pages

26 Andromedae

Article snapshot taken from[REDACTED] with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Star in the constellation Andromeda
26 Andromedae

A visual band light curve for 26 Andromedae, adapted from Zasche and Svoboda (2008)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
A
Right ascension 00 18 42.16888
Declination +43° 47′ 28.1082″
Apparent magnitude (V) 6.11
B
Right ascension 00 18 41.66160
Declination +43° 47′ 24.9776″
Apparent magnitude (V) 9.70
Characteristics
Evolutionary stage main sequence
Spectral type B8 V + F3 V
B−V color index −0.074±0.004
Variable type suspected
Astrometry
A
Radial velocity (Rv)+3.3 km/s
Proper motion (μ) RA: 23.328 mas/yr
Dec.: −2.755 mas/yr
Parallax (π)5.3927 ± 0.0192 mas
Distance605 ± 2 ly
(185.4 ± 0.7 pc)
Absolute magnitude (MV)0.02
B
Proper motion (μ) RA: 22.083 mas/yr
Dec.: −3.568 mas/yr
Parallax (π)5.4683 ± 0.0142 mas
Distance596 ± 2 ly
(182.9 ± 0.5 pc)
Absolute magnitude (MV)4.00
Details
A
Mass3.54±0.12 M
Radius3.76 R
Luminosity219 L
Surface gravity (log g)3.82 cgs
Temperature11,939 K
Rotational velocity (v sin i)18 km/s
Age95 Myr
B
Mass1.0 M
Radius1.2 R
Luminosity1.5 L
Surface gravity (log g)4.32 cgs
Temperature5,924 K
Age6.1 Gyr
Other designations
26 And, BD+42°48, HD 1438, HIP 1501, HR 70, SAO 36256, PPM 42805, WDS J00187+4347
Database references
SIMBADdata

26 Andromedae, abbreviated 26 And, is a binary star system in the constellation Andromeda. 26 Andromedae is the Flamsteed designation. It has a combined apparent visual magnitude of 6.10, which is near the lower limit of visibility to the naked eye. The distance to this system can be estimated from its annual parallax shift of 5.35 mas, which yields a distance of about 600 light years. At that distance, the visual magnitude of the stars is diminished from an extinction of 0.04 due to interstellar dust. The system is moving further from the Earth with a heliocentric radial velocity of +3.3 km/s.

The magnitude 6.11 primary, component A, is a B-type main-sequence star with a stellar classification of B8 V. The star has 3.54 times the mass of the Sun and 3.76 times the Sun's radius. It is around 95 million years old and is spinning with a projected rotational velocity of 18 km/s. 26 And is radiating 219 times the Sun's luminosity from its photosphere at an effective temperature of 11,939 K. It displays an infrared excess that suggests a circumstellar debris disk orbiting at a distance of 169.3 AU from the star with a temperature of 75 K.

The fainter secondary, component B, is a magnitude 9.70 star located 6.2 from the primary. It is an F-type main-sequence star with a class of F3 V that shows an unexplained long term variability.

One of the components of this system displays a slight photometric variation with a period of 3.16 days. This may be caused by pulsation or an ellipsoidal variation. This system's X-ray emission hasn't been detected yet, with an upper limit of Lx < 29.79 erg/s.

References

  1. ^ Zasche, P.; Svoboda, P. (May 2008), "The Unconfirmed Eclipsing Nature of V348 And and Detection of Variability of HD 1438", Information Bulletin on Variable Stars, 5827: 1, Bibcode:2008IBVS.5827....1Z.
  2. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  3. ^ Huélamo, N.; et al. (July 2000), "X-ray emission from Lindroos binary systems", Astronomy and Astrophysics, 359: 227–241, arXiv:astro-ph/0005348, Bibcode:2000A&A...359..227H.
  4. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  5. ^ Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics, 537: A120, arXiv:1201.2052, Bibcode:2012A&A...537A.120Z, doi:10.1051/0004-6361/201117691, S2CID 55586789.
  6. ^ Wyatt, M. C.; et al. (July 2007), "Steady State Evolution of Debris Disks around A Stars", The Astrophysical Journal, 663 (1): 365–382, arXiv:astro-ph/0703608, Bibcode:2007ApJ...663..365W, doi:10.1086/518404, S2CID 18883195.
  7. 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.
  8. Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1: B/gcvs. Bibcode:2009yCat....102025S.
  9. ^ Steenbrugge, K. C.; et al. (May 2003), "Radial velocities of early-type stars in the Perseus OB2 association", Astronomy and Astrophysics, 402 (2): 587–605, arXiv:astro-ph/0302428, Bibcode:2003A&A...402..587S, doi:10.1051/0004-6361:20030277, S2CID 15771155.
  10. 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.
  11. Lindroos, K. P. (May 1985), "A study of visual double stars with early type primaries. IV. Astrophysical data", Astronomy and Astrophysics, 60: 183–221, Bibcode:1985A&AS...60..183L.
  12. ^ Cotten, Tara H.; Song, Inseok (July 2016), "A Comprehensive Census of Nearby Infrared Excess Stars", The Astrophysical Journal Supplement Series, 225 (1): 24, arXiv:1606.01134, Bibcode:2016ApJS..225...15C, doi:10.3847/0067-0049/225/1/15, S2CID 118438871, 15.
  13. "26 And". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved September 25, 2018.

External links

Constellation of Andromeda
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Galaxies
Messier
NGC
Numbered
Other
Galaxy clusters
Astronomical events
Category
Categories:
26 Andromedae Add topic