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ADS 48

From Wikipedia, the free encyclopedia
Multiple star system with 7 stars in the constellation of Andromeda
ADS 48
Observation data
EpochJ2000      EquinoxJ2000
ConstellationAndromeda
ADS 48 A
Right ascension00h 05m 41.0219s[1]
Declination+45° 48′ 43.5452″[1]
Apparent magnitude (V)8.826[2]
ADS 48 B
Right ascension00h 05m 41.0028s[3]
Declination+45° 48′ 37.3535″[3]
Apparent magnitude (V)8.995[2]
ADS 48 F
Right ascension00h 05m 10.8892s[4]
Declination+45° 47′ 11.6395″[4]
Apparent magnitude (V)9.949[5]
Characteristics
ADS 48 A
Spectral typeK6V[6]
B−Vcolor index+1.344[2]
ADS 48 B
Spectral typeM0.5V[6]
B−Vcolor index+1.345[2]
ADS 48 F
Spectral typeM1V[5]
U−Bcolor index+1.18[7]
B−Vcolor index+1.50[7]
Astrometry
ADS 48 AB
Radial velocity (Rv)1.49±0.1[8] km/s
Proper motion (μ)RA: 887.48±1.02[9]mas/yr
Dec.: −152.02±1.04[9]mas/yr
Parallax (π)88.44±1.56 mas[9]
Distance36.9 ± 0.7 ly
(11.3 ± 0.2 pc)
ADS 48 F
Radial velocity (Rv)−0.39±0.09[8] km/s
Proper motion (μ)RA: 870.753±0.057[4] mas/yr
Dec.: −151.267±0.036[4] mas/yr
Parallax (π)86.9567 ± 0.0407 mas[4]
Distance37.51 ± 0.02 ly
(11.500 ± 0.005 pc)
Orbit[10]
PrimaryA
CompanionB
Period (P)509.65 ± 96.99yr
Semi-major axis (a)6.21 ± 0.77″
Eccentricity (e)0.22 ± 0.04
Inclination (i)54.9 ± 2.4°
Longitude of the node (Ω)13.5 ± 2.3°
Periastronepoch (T)2115.80 ± 123.47
Argument of periastron (ω)
(secondary)
267.2 ± 27.4°
Details
ADS 48 A
Mass0.50[10] M
ADS 48 B
Mass0.53[10] M
ADS 48 F
Radius0.618±0.027[5] R
Temperature3484±50[5] K
Rotation15.37(9)[11]days
Rotational velocity (v sin i)2.76[5] km/s
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
ADS 48 F:HIP 428,GJ 2,CCDM J00057+4548F,WDS J00057+4549F
Database references
SIMBADAB
A
B
F

ADS 48 is a multiple star system in theconstellation ofAndromeda consisting of 7 stars. The components, in order from A to G, haveapparent visual magnitudes of 8.826, 8.995,[2] 13.30,[12] 12.53, 11.68,[2] 9.949,[5] and 13.00.[13]

ADS 48A and ADS 48B are in orbital motion around each other while ADS 48F is acommon proper motion companion not gravitationally bound to the pair. The others are unassociated background stars, and component C could be a double star itself.[14] It has also been proposed the existence of an unseen companion of 0.05M.[10]

References

[edit]
  1. ^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.
  2. ^abcdefHøg, 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.
  3. ^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.
  4. ^abcdeBrown, 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. ^abcdefHoudebine, E. R. (2010)."Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars".Monthly Notices of the Royal Astronomical Society.407 (3):1657–1673.Bibcode:2010MNRAS.407.1657H.doi:10.1111/j.1365-2966.2010.16827.x.
  6. ^abTamazian, 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.
  7. ^abMermilliod, J.-C. (1986)."Compilation of Eggen's UBV data, transformed to UBV (unpublished)".Catalogue of Eggen's UBV Data.Bibcode:1986EgUBV........0M.
  8. ^abNidever, 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.
  9. ^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 entry
  10. ^abcdKiyaeva, 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.
  11. ^Díez Alonso, E.; et al. (January 2019)."CARMENES input catalogue of M dwarfs".Astronomy and Astrophysics.621 A126.arXiv:1810.03338.Bibcode:2019A&A...621A.126D.doi:10.1051/0004-6361/201833316.Vizier catalog entry
  12. ^"GSC 03246-01561".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved13 July 2013.
  13. ^"GSC 03246-00320".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved13 July 2013.
  14. ^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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