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Kappa1 Apodis

Kappa1 Apodis, Latinized from κ1 Apodis, is the Bayer designation for a binary star[3] system in the southern circumpolar constellation of Apus. Based upon parallax measurements, it is located roughly 1,060 light-years (325 parsecs) from Earth. The combined apparent visual magnitude of the system is 5.52,[2] indicating that this is a faint, naked eye star that can be viewed in dark suburban skies. It is moving away from the Sun with a radial velocity of +62 km/s.[5]

Kappa1 Apodis
Location of Kappa1 Apodis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension 15h 31m 30.82213s[1]
Declination −73° 23′ 22.5295″[1]
Apparent magnitude (V) 5.52[2]
Characteristics
Spectral type B1npe[3]
U−B color index −0.791[2]
B−V color index −0.128[2]
Variable type γ Cas[4]
Astrometry
Radial velocity (Rv)+62[5] km/s
Proper motion (μ) RA: +0.996[1] mas/yr
Dec.: −18.345[1] mas/yr
Parallax (π)3.0798 ± 0.0717 mas[1]
Distance1,060 ± 20 ly
(325 ± 8 pc)
Absolute magnitude (MV)−2.47[6]
Details
Mass12.0±0.3[7] M
Luminosity2,120[6] L
Surface gravity (log g)3.90[8] cgs
Temperature21,500[8] K
Age5.6±1.0[7] Myr
Other designations
κ1 Aps, CD−72°1139, CPD−72°1802, FK5 567, HD 137387, HIP 76013, HR 5730, SAO 257289[9]
Database references
SIMBADdata
A light curve for Kappa1 Apodis, plotted from TESS data[10]

This is a spectroscopic binary system with an orbital period of 0.6 days.[3] The combined spectrum matches a stellar classification of B1npe.[3] The 'e' suffix indicates that this is a Be star with emission lines in the spectrum. An 'n' means that the absorption lines in the spectrum are broadened from the Doppler effect as a result of rapid rotation. Finally, the 'p' shows some peculiarity in the spectrum. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to +5.61.

This is a runaway star with a peculiar velocity of 69.8±4.7 km/s.[7] Because it is a binary star system, it was most likely not turned into a runaway system as the result of a supernova explosion.[3] A companion star is a 12th magnitude orange K-type subgiant located at an angular separation of 27 arcseconds.

See also Edit

References Edit

  1. ^ a b c d e 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.
  2. ^ a b c d Gutierrez-Moreno, Adelina; Moreno, Hugo (June 1968), "A photometric investigation of the Scorpio-Centaurus association", Astrophysical Journal Supplement, 15: 459, Bibcode:1968ApJS...15..459G, doi:10.1086/190168.
  3. ^ a b c d e Jilinski, E.; et al. (September 2010), "A Dynamical Study of Suspected Runaway Stars as Traces of Past Supernova Explosions in the Region of the Scorpius-Centaurus OB Association", The Astrophysical Journal, 721 (1): 469–477, Bibcode:2010ApJ...721..469J, doi:10.1088/0004-637X/721/1/469.
  4. ^ 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, 1: 02025, Bibcode:2009yCat....102025S.
  5. ^ a b Evans, D. S. (June 20–24, 1966), "The Revision of the General Catalogue of Radial Velocities", in Batten, Alan Henry; Heard, John Frederick (eds.), Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30, vol. 30, University of Toronto: International Astronomical Union, p. 57, Bibcode:1967IAUS...30...57E.
  6. ^ a b 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.
  7. ^ a b c Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x, S2CID 118629873.
  8. ^ a b Soubiran, C.; Le Campion, J.-F.; Cayrel de Strobel, G.; Caillo, A. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv:1004.1069, Bibcode:2010A&A...515A.111S, doi:10.1051/0004-6361/201014247, S2CID 118362423.
  9. ^ "HR 5730", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2012-07-08.
  10. ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved 8 December 2021.

External links Edit

  • Image κ¹ Apodis

kappa1, apodis, latinized, from, apodis, bayer, designation, binary, star, system, southern, circumpolar, constellation, apus, based, upon, parallax, measurements, located, roughly, light, years, parsecs, from, earth, combined, apparent, visual, magnitude, sys. Kappa1 Apodis Latinized from k1 Apodis is the Bayer designation for a binary star 3 system in the southern circumpolar constellation of Apus Based upon parallax measurements it is located roughly 1 060 light years 325 parsecs from Earth The combined apparent visual magnitude of the system is 5 52 2 indicating that this is a faint naked eye star that can be viewed in dark suburban skies It is moving away from the Sun with a radial velocity of 62 km s 5 Kappa1 ApodisLocation of Kappa1 Apodis circled Observation dataEpoch J2000 Equinox J2000Constellation ApusRight ascension 15h 31m 30 82213s 1 Declination 73 23 22 5295 1 Apparent magnitude V 5 52 2 CharacteristicsSpectral type B1npe 3 U B color index 0 791 2 B V color index 0 128 2 Variable type g Cas 4 AstrometryRadial velocity Rv 62 5 km sProper motion m RA 0 996 1 mas yr Dec 18 345 1 mas yrParallax p 3 0798 0 0717 mas 1 Distance1 060 20 ly 325 8 pc Absolute magnitude MV 2 47 6 DetailsMass12 0 0 3 7 M Luminosity2 120 6 L Surface gravity log g 3 90 8 cgsTemperature21 500 8 KAge5 6 1 0 7 MyrOther designationsk1 Aps CD 72 1139 CPD 72 1802 FK5 567 HD 137387 HIP 76013 HR 5730 SAO 257289 9 Database referencesSIMBADdata A light curve for Kappa1 Apodis plotted from TESS data 10 This is a spectroscopic binary system with an orbital period of 0 6 days 3 The combined spectrum matches a stellar classification of B1npe 3 The e suffix indicates that this is a Be star with emission lines in the spectrum An n means that the absorption lines in the spectrum are broadened from the Doppler effect as a result of rapid rotation Finally the p shows some peculiarity in the spectrum It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude 5 43 to 5 61 This is a runaway star with a peculiar velocity of 69 8 4 7 km s 7 Because it is a binary star system it was most likely not turned into a runaway system as the result of a supernova explosion 3 A companion star is a 12th magnitude orange K type subgiant located at an angular separation of 27 arcseconds See also EditKappa ApodisReferences Edit a b c d e 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 amp A 674A 1G doi 10 1051 0004 6361 202243940 S2CID 244398875 Gaia DR3 record for this source at VizieR a b c d Gutierrez Moreno Adelina Moreno Hugo June 1968 A photometric investigation of the Scorpio Centaurus association Astrophysical Journal Supplement 15 459 Bibcode 1968ApJS 15 459G doi 10 1086 190168 a b c d e Jilinski E et al September 2010 A Dynamical Study of Suspected Runaway Stars as Traces of Past Supernova Explosions in the Region of the Scorpius Centaurus OB Association The Astrophysical Journal 721 1 469 477 Bibcode 2010ApJ 721 469J doi 10 1088 0004 637X 721 1 469 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 1 02025 Bibcode 2009yCat 102025S a b Evans D S June 20 24 1966 The Revision of the General Catalogue of Radial Velocities in Batten Alan Henry Heard John Frederick eds Determination of Radial Velocities and their Applications Proceedings from IAU Symposium no 30 vol 30 University of Toronto International Astronomical Union p 57 Bibcode 1967IAUS 30 57E a b 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 a b c Tetzlaff N Neuhauser R Hohle M M January 2011 A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun Monthly Notices of the Royal Astronomical Society 410 1 190 200 arXiv 1007 4883 Bibcode 2011MNRAS 410 190T doi 10 1111 j 1365 2966 2010 17434 x S2CID 118629873 a b Soubiran C Le Campion J F Cayrel de Strobel G Caillo A June 2010 The PASTEL catalogue of stellar parameters Astronomy and Astrophysics 515 A111 arXiv 1004 1069 Bibcode 2010A amp A 515A 111S doi 10 1051 0004 6361 201014247 S2CID 118362423 HR 5730 SIMBAD Centre de donnees astronomiques de Strasbourg retrieved 2012 07 08 MAST Barbara A Mikulski Archive for Space Telescopes Space Telescope Science Institute retrieved 8 December 2021 External links EditImage k Apodis Retrieved from https en wikipedia org w index php title Kappa1 Apodis amp oldid 1171337063, wikipedia, wiki, book, books, library,

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