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13 Sagittae

13 Sagittae is a single[10] star in the northern constellation of Sagitta. The designation comes from the star catalogue of John Flamsteed, first published in 1712. It can be viewed with the naked eye, having an apparent visual magnitude of 5.33.[1] Based upon an annual parallax shift of 5.94 mas as seen from Earth's orbit, it is located at a distance of around 170 parsecs (550 ly). It is moving closer to the Sun with a heliocentric radial velocity of −17.56 km/s.[5]

13 Sagittae

A visual band light curve for VZ Sagittae, plotted from data published by Tabur et al. (2009)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Sagitta
Right ascension 20h 00m 03.30846s[2]
Declination +17° 30′ 59.4373″[2]
Apparent magnitude (V) 5.33[1]
Characteristics
Spectral type M4 III[1]
B−V color index 1.576±0.010[3]
Variable type semiregular[4]
Astrometry
Radial velocity (Rv)−17.56±0.33[5] km/s
Proper motion (μ) RA: +49.424[2] mas/yr
Dec.: +2.738[2] mas/yr
Parallax (π)5.94 ± 0.36 mas[2]
Distance550 ± 30 ly
(170 ± 10 pc)
Absolute magnitude (MV)−2.12[3]
Details
Radius60[6] R
Luminosity2173.57[3] L
Surface gravity (log g)3.00[7] cgs
Temperature3,844±251[8] K
Other designations
13 Sge, VZ Sge, BD+17° 4183, HD 189577, HIP 98438, HR 7645, SAO 105522, WDS J20001+1731C[9]
Database references
SIMBADdata
Pulsation Cycles[1]
Period
(days)
Amplitude
(magnitude)
36.5 0.082
39.2 0.043
51.4 0.031
65.2 0.030

This is an evolved red giant with a stellar classification of M4 III[1] – a star that has used up its core hydrogen and has expanded – and is currently on the asymptotic giant branch.[7] Classified as a semiregular variable and given the variable star designation VZ Sagittae, it varies between apparent magnitudes 5.27 and 5.57.[4] The measured angular diameter, after correction for limb darkening, is 3.3±1.1 mas.[11] At its estimated distance, this yields a physical size of about 60 times the radius of the Sun.[6]

There is a magnitude 9.96 companion located at an angular separation of 112.6 arcseconds along a position angle of 297°, as of 2013.[12] Designated HD 351107, this is a class F0 star.[13]

References

  1. ^ a b c d e f Tabur, V.; et al. (December 2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society. 400 (4): 1945–1961. arXiv:0908.3228. Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x. S2CID 15358380.
  2. ^ a b c d e 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.
  3. ^ a b c 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.
  4. ^ a b VSX (25 August 2009). "VZ Sagittae". AAVSO Website. American Association of Variable Star Observers. Retrieved 4 January 2015.
  5. ^ a b Famaey, B.; et al. (January 2005). "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters". Astronomy and Astrophysics. 430: 165–186. arXiv:astro-ph/0409579. Bibcode:2005A&A...430..165F. doi:10.1051/0004-6361:20041272. S2CID 17804304.
  6. ^ a b Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by:
     
  7. ^ a b Ortiz, Roberto; Guerrero, Martín A. (2016). "Ultraviolet emission from main-sequence companions of AGB stars". Monthly Notices of the Royal Astronomical Society. 461 (3): 3036. arXiv:1606.09086. Bibcode:2016MNRAS.461.3036O. doi:10.1093/mnras/stw1547. S2CID 118619933.
  8. ^ Soubiran, C.; et al. (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. ^ "13 Sge". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-02-28.
  10. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  11. ^ Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode:2005A&A...431..773R, doi:10.1051/0004-6361:20042039
  12. ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ....122.3466M, doi:10.1086/323920
  13. ^ Nesterov, V. V.; et al. (1995). "The Henry Draper Extension Charts: A catalogue of accurate positions, proper motions, magnitudes and spectral types of 86933 stars". Astronomy and Astrophysics. 110: 367. Bibcode:1995A&AS..110..367N.

sagittae, single, star, northern, constellation, sagitta, designation, comes, from, star, catalogue, john, flamsteed, first, published, 1712, viewed, with, naked, having, apparent, visual, magnitude, based, upon, annual, parallax, shift, seen, from, earth, orb. 13 Sagittae is a single 10 star in the northern constellation of Sagitta The designation comes from the star catalogue of John Flamsteed first published in 1712 It can be viewed with the naked eye having an apparent visual magnitude of 5 33 1 Based upon an annual parallax shift of 5 94 mas as seen from Earth s orbit it is located at a distance of around 170 parsecs 550 ly It is moving closer to the Sun with a heliocentric radial velocity of 17 56 km s 5 13 SagittaeA visual band light curve for VZ Sagittae plotted from data published by Tabur et al 2009 1 Observation dataEpoch J2000 Equinox J2000Constellation SagittaRight ascension 20h 00m 03 30846s 2 Declination 17 30 59 4373 2 Apparent magnitude V 5 33 1 CharacteristicsSpectral type M4 III 1 B V color index 1 576 0 010 3 Variable type semiregular 4 AstrometryRadial velocity Rv 17 56 0 33 5 km sProper motion m RA 49 424 2 mas yr Dec 2 738 2 mas yrParallax p 5 94 0 36 mas 2 Distance550 30 ly 170 10 pc Absolute magnitude MV 2 12 3 DetailsRadius60 6 R Luminosity2173 57 3 L Surface gravity log g 3 00 7 cgsTemperature3 844 251 8 KOther designations13 Sge VZ Sge BD 17 4183 HD 189577 HIP 98438 HR 7645 SAO 105522 WDS J20001 1731C 9 Database referencesSIMBADdata Pulsation Cycles 1 Period days Amplitude magnitude 36 5 0 08239 2 0 04351 4 0 03165 2 0 030This is an evolved red giant with a stellar classification of M4 III 1 a star that has used up its core hydrogen and has expanded and is currently on the asymptotic giant branch 7 Classified as a semiregular variable and given the variable star designation VZ Sagittae it varies between apparent magnitudes 5 27 and 5 57 4 The measured angular diameter after correction for limb darkening is 3 3 1 1 mas 11 At its estimated distance this yields a physical size of about 60 times the radius of the Sun 6 There is a magnitude 9 96 companion located at an angular separation of 112 6 arcseconds along a position angle of 297 as of 2013 12 Designated HD 351107 this is a class F0 star 13 References Edit a b c d e f Tabur V et al December 2009 Long term photometry and periods for 261 nearby pulsating M giants Monthly Notices of the Royal Astronomical Society 400 4 1945 1961 arXiv 0908 3228 Bibcode 2009MNRAS 400 1945T doi 10 1111 j 1365 2966 2009 15588 x S2CID 15358380 a b c d e 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 a b c 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 VSX 25 August 2009 VZ Sagittae AAVSO Website American Association of Variable Star Observers Retrieved 4 January 2015 a b Famaey B et al January 2005 Local kinematics of K and M giants from CORAVEL Hipparcos Tycho 2 data Revisiting the concept of superclusters Astronomy and Astrophysics 430 165 186 arXiv astro ph 0409579 Bibcode 2005A amp A 430 165F doi 10 1051 0004 6361 20041272 S2CID 17804304 a b Lang Kenneth R 2006 Astrophysical formulae Astronomy and astrophysics library vol 1 3rd ed Birkhauser ISBN 3 540 29692 1 The radius R is given by 2 R 168 4 3 3 10 3 AU 0 0046491 AU R 119 5 R displaystyle begin aligned 2 cdot R amp frac 168 4 cdot 3 3 cdot 10 3 text AU 0 0046491 text AU R bigodot amp approx 119 5 cdot R bigodot end aligned a b Ortiz Roberto Guerrero Martin A 2016 Ultraviolet emission from main sequence companions of AGB stars Monthly Notices of the Royal Astronomical Society 461 3 3036 arXiv 1606 09086 Bibcode 2016MNRAS 461 3036O doi 10 1093 mnras stw1547 S2CID 118619933 Soubiran C et al 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 13 Sge SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 2018 02 28 Eggleton P P Tokovinin A A September 2008 A catalogue of multiplicity among bright stellar systems Monthly Notices of the Royal Astronomical Society 389 2 869 879 arXiv 0806 2878 Bibcode 2008MNRAS 389 869E doi 10 1111 j 1365 2966 2008 13596 x S2CID 14878976 Richichi A et al February 2005 CHARM2 An updated Catalog of High Angular Resolution Measurements Astronomy and Astrophysics 431 2 773 777 Bibcode 2005A amp A 431 773R doi 10 1051 0004 6361 20042039 Mason B D et al 2014 The Washington Visual Double Star Catalog The Astronomical Journal 122 6 3466 Bibcode 2001AJ 122 3466M doi 10 1086 323920 Nesterov V V et al 1995 The Henry Draper Extension Charts A catalogue of accurate positions proper motions magnitudes and spectral types of 86933 stars Astronomy and Astrophysics 110 367 Bibcode 1995A amp AS 110 367N Retrieved from https en wikipedia org w index php title 13 Sagittae amp oldid 1079520975, wikipedia, wiki, book, books, library,

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