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ADS 48

From Wikipedia, the free encyclopedia
Triple star system in the constellation of Andromeda
ADS 48
Observation data
EpochJ2000      EquinoxJ2000
ConstellationAndromeda[1]
ADS 48 A
Right ascension00h 05m 41.0219s[2]
Declination+45° 48′ 43.545″[2]
Apparent magnitude (V)8.826[3]
ADS 48 B
Right ascension00h 05m 41.0028s[4]
Declination+45° 48′ 37.354″[4]
Apparent magnitude (V)8.995[3]
Characteristics
ADS 48 A
Spectral typeK6V[5]
B−Vcolor index+1.344[3]
ADS 48 B
Spectral typeM0.5V[5]
B−Vcolor index+1.345[3]
Astrometry
Radial velocity (Rv)1.49±0.1[6] km/s
Proper motion (μ)RA: 887.48±1.02[7]mas/yr
Dec.: −152.02±1.04[7]mas/yr
Parallax (π)88.44±1.56 mas[7]
Distance36.9 ± 0.7 ly
(11.3 ± 0.2 pc)
Absolute magnitude (MV)+7.93[1]
Orbit[8]
Period (P)557±120 yr
Semi-major axis (a)74±10 AU
Eccentricity (e)0.19±0.08
Inclination (i)54.3±2.3°
Longitude of the node (Ω)12.5±2.8°
Periastronepoch (T)2110±30
Argument of periastron (ω)
(secondary)
256±31°
Details
ADS 48 A
Mass0.50[9] M
ADS 48 B
Mass0.53[9] M
Other designations
HD 38,HIP 473,GJ 4,CCDM J00057+4548AB,WDS J00057+4549AB
ADS 48 A:HD 38A,SAO 36046,GC 71,GJ 4 A,CCDM J00057+4548A,WDS J00057+4549A
ADS 48 B:HD 38B,SAO 36048,GC 72,GJ 4 B,CCDM J00057+4548B,WDS J00057+4549B
Database references
SIMBADAB
A
B

ADS 48 is abinary system in theconstellation ofAndromeda.

The components haveapparent visual magnitudes of 8.826 and 8.995.[3] Component A is aK-type main-sequence star, while component B is anM-type main-sequence star (red dwarf).[5] The stars are orbiting with aperiod of 550 years and a separation of74 AU.[8]

Multiple stars lie close to ADS 48 in the line of sight, and have been considered components C, D and E of the system, but are background objects. ADS 48 F (Gliese 2) is at a similar distance from the pair and share similarproper motions, but is moving faster than theescape velocity of the pair and thus is not gravitationally bound.[10] The existence of an unseen companion of 0.05 M has also been proposed,[9] but this was refuted.[8]

References

[edit]
  1. ^abAnderson, 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. XHIP record for this object atVizieR.
  2. ^abBrown, 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. Gaia DR2 record for this source atVizieR.
  3. ^abcdeHøg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (2000). "The Tycho-2 catalogue of the 2.5 million brightest stars".Astronomy & Astrophysics.355:L27–L30.Bibcode:2000A&A...355L..27H.
  4. ^abBrown, 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. Gaia DR2 record for this source atVizieR.
  5. ^abcTamazian, Vakhtang S.; Docobo, José A.; Melikian, Norair D.; Karapetian, Arthur A. (2006)."MK Classification and Dynamical Masses for Late-Type Visual Binaries".Publications of the Astronomical Society of the Pacific.118 (844): 814.Bibcode:2006PASP..118..814T.doi:10.1086/504881.
  6. ^Nidever, David L.; Marcy, Geoffrey W.; Butler, R. Paul; Fischer, Debra A.; Vogt, Steven S. (2002). "Radial Velocities for 889 Late-Type Stars".The Astrophysical Journal Supplement Series.141 (2):503–522.arXiv:astro-ph/0112477.Bibcode:2002ApJS..141..503N.doi:10.1086/340570.S2CID 51814894.
  7. ^abcvan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction".Astronomy and Astrophysics.474 (2):653–664.arXiv:0708.1752.Bibcode:2007A&A...474..653V.doi:10.1051/0004-6361:20078357.S2CID 18759600.Vizier catalog entryArchived 2019-04-02 at theWayback Machine
  8. ^abcKiyaeva, O. V.; Zhuchkov, R. Ya; Izmailov, I. S. (2021). "Investigation of relative motion in the triple system ADS 48 on the basis of Gaia DR2 and Pulkovo 26-inch refractor observations".Astronomical and Astrophysical Transactions.32 (2):89–98.Bibcode:2021A&AT...32...89K.ISSN 1055-6796.
  9. ^abcKiyaeva, O. V. (2001). "An astrometric study of the triple star ADS 48".Astronomy Letters.21 (6):391–397.Bibcode:2001AstL...27..391K.doi:10.1134/1.1374678.S2CID 121012446.
  10. ^Cvetković, Z.; et al. (2012)."System ADS 48: Visual Binary or Multiple System".The Astronomical Journal.144 (3) 80.Bibcode:2012AJ....144...80C.doi:10.1088/0004-6256/144/3/80.S2CID 120045704.
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