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Epsilon Pavonis

Epsilon Pavonis, Latinized from ε Pavonis, is a single,[9] white-hued star in the constellation Pavo. It can be viewed with the naked eye, having an apparent visual magnitude of 3.97.[2] The annual parallax shift of 31.04[1] mas provides a distance estimate of 105 light years from the Sun. This star is a member of the proposed Argus Association, a young moving group of more than 60 stars associated with the IC 2391 cluster.[10] Epsilon Pavonis is moving closer to the Sun with a radial velocity of −6.7 km/s.[4]

ε Pavonis
Location of ε Pavonis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pavo
Right ascension 20h 00m 35.55558s[1]
Declination −72° 54′ 37.8198″[1]
Apparent magnitude (V) 3.97[2]
Characteristics
Spectral type A0 Va[2]
U−B color index −0.05[3]
B−V color index −0.03[2]
Astrometry
Radial velocity (Rv)−6.7±0.7[4] km/s
Proper motion (μ) RA: +81.78[1] mas/yr
Dec.: −132.16[1] mas/yr
Parallax (π)31.04 ± 0.17 mas[1]
Distance105.1 ± 0.6 ly
(32.2 ± 0.2 pc)
Absolute magnitude (MV)1.43[2]
Details
Mass2.2[5] M
Radius1.74[6] R
Luminosity32[7] L
Surface gravity (log g)4.32±0.02[6] cgs
Temperature10,440[8] K
Rotational velocity (v sin i)85[7] km/s
Age27[6] Myr
Other designations
ε Pav, CPD−73° 2086, FK5 748, GC 27631, HD 188228, HIP 98495, HR 7590, SAO 257757
Database references
SIMBADdata

With a stellar classification of A0 Va,[2] Epsilon Pavonis is an ordinary A-type main-sequence star that is generating energy through hydrogen fusion at its core. It is just 27[6] million years old with a projected rotational velocity of 85[7] km/s. The star has 2.2[5] times the mass of the Sun and 1.74[6] the Sun's radius. It is radiating 32[7] times the Sun's luminosity from its photosphere at an effective temperature of 10,440 K.[8]

References edit

  1. ^ a b c d e f Van 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
  2. ^ a b c d e f 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. Vizier catalog entry
  3. ^ Mermilliod, J. C. (2006). "VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991)". VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie. 2168. Bibcode:2006yCat.2168....0M.Vizier catalog entry
  4. ^ a b Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  5. ^ a b Tetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (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. Vizier catalog entry
  6. ^ a b c d e Gerbaldi, M.; et al. (June 1999), "Search for reference A0 dwarf stars: Masses and luminosities revisited with HIPPARCOS parallaxes", Astronomy and Astrophysics Supplement, 137 (2): 273–292, Bibcode:1999A&AS..137..273G, doi:10.1051/aas:1999248.
  7. ^ a b c d Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars". Astronomy & Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. S2CID 55586789. Vizier catalog entry
  8. ^ a b David, Trevor J.; Hillenbrand, Lynne A. (2015). "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets". The Astrophysical Journal. 804 (2): 146. arXiv:1501.03154. Bibcode:2015ApJ...804..146D. doi:10.1088/0004-637X/804/2/146. S2CID 33401607. Vizier catalog entry
  9. ^ Eggleton, P. P.; Tokovinin, A. A. (2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  10. ^ Zuckerman, B.; et al. (May 2011). "The Tucana/Horologium, Columba, AB Doradus, and Argus Associations: New Members and Dusty Debris Disks". The Astrophysical Journal. 732 (2): 19. arXiv:1104.0284. Bibcode:2011ApJ...732...61Z. doi:10.1088/0004-637X/732/2/61. S2CID 62797470. 61.

epsilon, pavonis, latinized, from, pavonis, single, white, hued, star, constellation, pavo, viewed, with, naked, having, apparent, visual, magnitude, annual, parallax, shift, provides, distance, estimate, light, years, from, this, star, member, proposed, argus. Epsilon Pavonis Latinized from e Pavonis is a single 9 white hued star in the constellation Pavo It can be viewed with the naked eye having an apparent visual magnitude of 3 97 2 The annual parallax shift of 31 04 1 mas provides a distance estimate of 105 light years from the Sun This star is a member of the proposed Argus Association a young moving group of more than 60 stars associated with the IC 2391 cluster 10 Epsilon Pavonis is moving closer to the Sun with a radial velocity of 6 7 km s 4 e PavonisLocation of e Pavonis circled Observation dataEpoch J2000 Equinox J2000 Constellation Pavo Right ascension 20h 00m 35 55558s 1 Declination 72 54 37 8198 1 Apparent magnitude V 3 97 2 Characteristics Spectral type A0 Va 2 U B color index 0 05 3 B V color index 0 03 2 AstrometryRadial velocity Rv 6 7 0 7 4 km sProper motion m RA 81 78 1 mas yr Dec 132 16 1 mas yrParallax p 31 04 0 17 mas 1 Distance105 1 0 6 ly 32 2 0 2 pc Absolute magnitude MV 1 43 2 DetailsMass2 2 5 M Radius1 74 6 R Luminosity32 7 L Surface gravity log g 4 32 0 02 6 cgsTemperature10 440 8 KRotational velocity v sin i 85 7 km sAge27 6 Myr Other designationse Pav CPD 73 2086 FK5 748 GC 27631 HD 188228 HIP 98495 HR 7590 SAO 257757 Database referencesSIMBADdata With a stellar classification of A0 Va 2 Epsilon Pavonis is an ordinary A type main sequence star that is generating energy through hydrogen fusion at its core It is just 27 6 million years old with a projected rotational velocity of 85 7 km s The star has 2 2 5 times the mass of the Sun and 1 74 6 the Sun s radius It is radiating 32 7 times the Sun s luminosity from its photosphere at an effective temperature of 10 440 K 8 References edit a b c d e f Van Leeuwen F 2007 Validation of the new Hipparcos reduction Astronomy and Astrophysics 474 2 653 664 arXiv 0708 1752 Bibcode 2007A amp A 474 653V doi 10 1051 0004 6361 20078357 S2CID 18759600 Vizier catalog entry a b c d e f 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 Vizier catalog entry Mermilliod J C 2006 VizieR Online Data Catalog Homogeneous Means in the UBV System Mermilliod 1991 VizieR On line Data Catalog II 168 Originally Published in Institut d Astronomie 2168 Bibcode 2006yCat 2168 0M Vizier catalog entry a b Gontcharov G A 2006 Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system Astronomy Letters 32 11 759 771 arXiv 1606 08053 Bibcode 2006AstL 32 759G doi 10 1134 S1063773706110065 S2CID 119231169 a b Tetzlaff N Neuhauser R Hohle M M 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 Vizier catalog entry a b c d e Gerbaldi M et al June 1999 Search for reference A0 dwarf stars Masses and luminosities revisited with HIPPARCOS parallaxes Astronomy and Astrophysics Supplement 137 2 273 292 Bibcode 1999A amp AS 137 273G doi 10 1051 aas 1999248 a b c d Zorec J Royer F 2012 Rotational velocities of A type stars Astronomy amp Astrophysics 537 A120 arXiv 1201 2052 Bibcode 2012A amp A 537A 120Z doi 10 1051 0004 6361 201117691 S2CID 55586789 Vizier catalog entry a b David Trevor J Hillenbrand Lynne A 2015 The Ages of Early Type Stars Stromgren Photometric Methods Calibrated Validated Tested and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets The Astrophysical Journal 804 2 146 arXiv 1501 03154 Bibcode 2015ApJ 804 146D doi 10 1088 0004 637X 804 2 146 S2CID 33401607 Vizier catalog entry Eggleton P P Tokovinin A A 2008 A catalogue of multiplicity among bright stellar systems Monthly Notices of the Royal Astronomical Society 389 2 869 arXiv 0806 2878 Bibcode 2008MNRAS 389 869E doi 10 1111 j 1365 2966 2008 13596 x S2CID 14878976 Zuckerman B et al May 2011 The Tucana Horologium Columba AB Doradus and Argus Associations New Members and Dusty Debris Disks The Astrophysical Journal 732 2 19 arXiv 1104 0284 Bibcode 2011ApJ 732 61Z doi 10 1088 0004 637X 732 2 61 S2CID 62797470 61 Retrieved from https en wikipedia org w index php title Epsilon Pavonis amp oldid 1124781669, wikipedia, wiki, book, books, library,

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