13 Vulpeculae

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13 Vulpeculae
Vulpecula constellation map.svg
Red circle.svg
Location of 13 Vulpeculae (circled)
Observation data
Epoch J2000       Equinox J2000
Constellation Vulpecula
13 Vulpeculae A
Right ascension 19h 53m 27.6957s [1]
Declination 24° 04′ 46.608″ [1]
Apparent magnitude  (V)4.584±0.008 [2]
13 Vulpeculae B
Right ascension 19h 53m 27.6102s [3]
Declination 24° 04′ 46.077″ [3]
Characteristics
Spectral type B9.5III [4]
Apparent magnitude  (U)4.404±0.012 [2]
Apparent magnitude  (B)4.536±0.010 [2]
Astrometry
13 Vulpeculae A
Radial velocity (Rv)−28.10 [5]  km/s
Proper motion (μ)RA: 22.325±0.065 [1]   mas/yr
Dec.: 36.510±0.072 [1]   mas/yr
Parallax (π)9.6342 ± 0.0902  mas [1]
Distance 339 ± 3  ly
(103.8 ± 1.0  pc)
Absolute magnitude  (MV)−0.48 [4]
13 Vulpeculae B
Proper motion (μ)RA: 14.037±0.135 [3]   mas/yr
Dec.: 32.954±0.131 [3]   mas/yr
Parallax (π)9.8828 ± 0.1524  mas [3]
Distance 330 ± 5  ly
(101 ± 2  pc)
Orbit [6]
Period (P)615.25±104.12 yr
Semi-major axis (a)1.555±0.241″
Eccentricity (e)0.079±0.042
Inclination (i)85.9±1.5°
Longitude of the node (Ω)68.1±0.3°
Periastron epoch (T)2027.82±94.79
Argument of periastron (ω)
(secondary)		169.7±4.4°
Details
13 Vul A
Radius 1.3 [7]   R☉
Luminosity 180 [4]   L☉
Temperature 8,801 [8]   K
Metallicity [Fe/H]−0.11 [4]   dex
Rotational velocity (v sin i)45.0 [9]  km/s
Other designations
13 Vul, BD+23°3820, GC  27544, HD  188260, HIP  97886, HR  7592, SAO  87883, CCDM J19535+2405AB, WDS J19535+2405AB, 2MASS J19532768+2404464 [10]
Database references
SIMBAD data

13 Vulpeculae is a blue giant with a stellar classification of class B9.5III [4] in the northern constellation Vulpecula. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.57 [4] and it is approximately 339 light years away from the Sun based on parallax. The star is radiating 180 [4] times the luminosity of the Sun from its photosphere at an effective temperature of 8,801 K. [8]

There is one reported companion, designated component B, with a magnitude of 7.37, an orbital period of roughly 615 years, and an angular separation of 1.55″ . [11] The system is moving closer to the Earth with a heliocentric radial velocity of −28 km/s. [5]

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<span class="mw-page-title-main">23 Vulpeculae</span> Star in the constellation Vulpecula

23 Vulpeculae is a triple star system in the northern constellation of Vulpecula. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.52 and it is located approximately 327 light years away from the Sun based on parallax. The system is moving further from the Earth with a heliocentric radial velocity of +1.47 km/s.

<span class="mw-page-title-main">15 Vulpeculae</span> Star in the constellation Vulpecula

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<span class="mw-page-title-main">1 Vulpeculae</span> Star in the constellation Vulpecula

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<span class="mw-page-title-main">12 Vulpeculae</span> Star in the constellation Vulpecula

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<span class="mw-page-title-main">V381 Cephei</span> Triple star system in the constellation Cepheus

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<span class="mw-page-title-main">Zeta Chamaeleontis</span> Variable star in the constellation Chamaeleon

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<span class="mw-page-title-main">1 Camelopardalis</span> Double star system in the constellation Camelopardalis

1 Camelopardalis is a double star system in the constellation Camelopardalis. Its combined apparent magnitude is 5.56 and it is approximately 800 parsecs (2,600 ly) away.

<span class="mw-page-title-main">HD 102839</span> Star in the constellation Musca

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<span class="mw-page-title-main">Pi Pavonis</span> Astrometric binary star system in the constellation Pavo

π Pavonis, Latinized as Pi Pavonis, is a candidate astrometric binary star system in the constellation Pavo. It is a white-hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.33. The distance to this object is 130 light years based on parallax, but it is drifting closer to the Sun with a radial velocity of −15.6 km/s.

Phi<sup>1</sup> Pavonis Single star in the constellation Pavo

Phi1 Pavonis, latinized from φ1 Pavonis, is a single star in the southern constellation of Pavo. It has a yellow-white hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.75. The star is located at a distance of approximately 92 light years away based on parallax. It is drifting closer to the Sun with a radial velocity of −20 km/s.

<span class="mw-page-title-main">QZ Puppis</span> Star in the constellation Puppis

QZ Puppis is a class B2.5V star in the constellation Puppis. Its apparent magnitude is 4.5 and it is approximately 650 light years away based on parallax.

<span class="mw-page-title-main">1 Puppis</span> Star in the constellation Puppis

1 Puppis is a single star in the southern constellation of Puppis. It lies in the northern part of the constellation at a distance of about 790 ly, east of Aludra in Canis Major and just north of the white supergiant, 3 Puppis. This object is visible to the naked eye as a faint, red-hued star with an apparent visual magnitude of 4.59. It is moving further from the Earth with a heliocentric radial velocity of +32.4 km/s.

<span class="mw-page-title-main">HD 59890</span> Star in the constellation Puppis

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<span class="mw-page-title-main">HD 54893</span> Star in the constellation Puppis

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HD 155448 is a quintuple star system consisting of 5 young B-type stars. With an apparent magnitude of 8.72, it is too dim to be visible with the naked eye.

36 Camelopardalis is a single star in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye as a dim point of light with an apparent visual magnitude of +5.3. Parallax measurements provide a distance estimate of approximately 710 light years away from the Sun, and it is drifting away from the Earth with a radial velocity of −1.15 km/s.

<span class="mw-page-title-main">HD 33541</span> Spectroscopic binary; Camelopardalis

HD 33541, also known as HR 1683, is a white-hued star located in the northern circumpolar constellation Camelopardalis. It has an apparent magnitude of 5.83, making it faintly visible to the naked eye. Gaia DR3 parallax measurements imply a distance of 358 light years and it is currently receding with a heliocentric radial velocity of 9.9 km/s. At its current distance HD 33541's brightness is diminished by 0.16 magnitudes due to interstellar extinction and it has an absolute magnitude of +0.58.

References

  1. 1 2 3 4 5 Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv: 2012.01533 . Bibcode:2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657 . S2CID   227254300. (Erratum:  doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. 1 2 3 Harmanec, P.; et al. (2020). "A new study of the spectroscopic binary 7 Vul with a Be star primary". Astronomy and Astrophysics. 639. Table A.1. arXiv: 2005.11089 . Bibcode:2020A&A...639A..32H. doi:10.1051/0004-6361/202037964. S2CID   218862853.
  3. 1 2 3 4 5 Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv: 2012.01533 . Bibcode:2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657 . S2CID   227254300. (Erratum:  doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  4. 1 2 3 4 5 6 7 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
  5. 1 2 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.
  6. ↑ Hartkopf, W. I.; et al. (June 30, 2006), Sixth Catalog of Orbits of Visual Binary Stars, United States Naval Observatory, archived from the original on 2017-08-01, retrieved 2017-06-02.
  7. ↑ Pasinetti Fracassini, L. E.; et al. (February 2001). "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)". Astronomy and Astrophysics. 367 (2) (Third ed.): 521–524. arXiv: astro-ph/0012289 . Bibcode:2001A&A...367..521P. doi:10.1051/0004-6361:20000451. S2CID   425754.
  8. 1 2 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental parameters and infrared excesses of Hipparcos stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–357. arXiv: 1208.2037 . Bibcode:2012MNRAS.427..343M. doi: 10.1111/j.1365-2966.2012.21873.x . S2CID   118665352. Vizier catalog entry
  9. ↑ Glebocki, R.; Gnacinski, P. (2005). "VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005)". VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G. 3244. Bibcode:2005yCat.3244....0G. Vizier catalog entry
  10. ↑ "13 Vul". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2019-03-15.
  11. ↑ Malkov, O. Yu.; Tamazian, V. S.; Docobo, J. A.; Chulkov, D. A. (2012). "Dynamical masses of a selected sample of orbital binaries". Astronomy & Astrophysics. 546: A69. Bibcode:2012A&A...546A..69M. doi: 10.1051/0004-6361/201219774 . Vizier catalog entry
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