13 Delphini
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Delphinus |
A | |
Right ascension | 20h 47m 48.3330s[1] |
Declination | +06° 00′ 29.551″[1] |
Apparent magnitude (V) | 5.66[2] |
B | |
Right ascension | 20h 47m 48.3012s[1] |
Declination | +06° 00′ 28.127″[1] |
Apparent magnitude (V) | 8.51[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | A0 V[4] |
U−B color index | −0.09[5] |
B−V color index | −0.01[5] |
Astrometry | |
Radial velocity (Rv) | −7±4.3[6] km/s |
Absolute magnitude (MV) | −0.01[7] |
A | |
Proper motion (μ) | RA: +8.255 mas/yr[1] Dec.: −13.162 mas/yr[1] |
Parallax (π) | 6.9265 ± 0.0489 mas[1] |
Distance | 471 ± 3 ly (144 ± 1 pc) |
B | |
Proper motion (μ) | RA: +5.663 mas/yr[8] Dec.: −12.280 mas/yr[8] |
Parallax (π) | 6.6697 ± 0.0989 mas[8] |
Distance | 489 ± 7 ly (150 ± 2 pc) |
Details | |
Mass | 2.51+0.31 −0.36[9] M☉ |
Radius | 3.7±0.4[9] R☉ |
Luminosity | 119+20 −17[3] L☉ |
Surface gravity (log g) | 3.69+0.61 −0.69[9] cgs |
Temperature | 9,840+91 −90[3] K |
Metallicity [Fe/H] | 0.00[10] dex |
Rotational velocity (v sin i) | 170[11] km/s |
Age | 307[10] Myr |
Other designations | |
Database references | |
SIMBAD | data |
13 Delphini is a binary star[2] in the equatorial constellation Delphinus, with a combined apparent magnitude of 5.64.[12] The system is located at a distance of 471 light years but is approaching the Solar System with a heliocentric radial velocity of about −7 km/s.[6]
13 Delphini A has an apparent magnitude of 5.66, while its companion has an apparent magnitude of 8.51.[2] As of 2016, the pair have a separation of 1.5″ located at a position angle of 200°.[13]
13 Delphini has a blended stellar classification of A0 V,[4] indicating that it is an ordinary A-type main-sequence star. However, when the components are analysed individually, the primary star is given a class of B9V.[14] It has 2.51 times the mass of the Sun[9] and has an effective temperature of 9,840 K.[3] However, the star is large for its class, having a radius almost 4 times that of the Sun[9] and a luminosity 119 times greater.[3] This is due to 13 Delphini having completed 86.1% of its main sequence lifetime[3] and has led one source to classify it as a subgiant instead.[15] It spins rapidly with a projected rotational velocity of 170 km/s[11] and has an age of 307 million years.[10]
References
- ^ a b c d e f 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.
- ^ a b c d 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.
- ^ a b c d e f Zorec, J.; Royer, F. (January 2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. ISSN 0004-6361. S2CID 55586789.
- ^ a b Paunzen, E.; Duffee, B.; Heiter, U.; Kuschnig, R.; Weiss, W. W. (July 2001). "A spectroscopic survey for λ Bootis stars". Astronomy & Astrophysics. 373 (2). EDP Sciences: 625–632. Bibcode:2001A&A...373..625P. doi:10.1051/0004-6361:20010630. ISSN 0004-6361.
- ^ a b Cousins, A. W. J. (1971). "Photometric standard stars". Royal Observatory Annals. 7: 86. Bibcode:1971ROAn....7.....C.
- ^ a b Gontcharov, G. A. (November 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. ISSN 1063-7737. S2CID 119231169.
- ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. ISSN 1063-7737. S2CID 255204555.
- ^ a b 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.
- ^ a b c d e Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256.
- ^ a b c Gontcharov, G. A. (December 2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. ISSN 0320-0108. S2CID 255201789.
- ^ a b Royer, F.; Zorec, J.; Gómez, A. E. (23 November 2006). "Rotational velocities of A-type stars". Astronomy & Astrophysics. 463 (2): 671–682. arXiv:astro-ph/0610785. Bibcode:2007A&A...463..671R. doi:10.1051/0004-6361:20065224. eISSN 1432-0746. ISSN 0004-6361.
- ^ Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (2002-03-01). "The Tycho double star catalogue". Astronomy and Astrophysics. 384: 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822. ISSN 0004-6361.
- ^ Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (December 2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466–3471. Bibcode:2001AJ....122.3466M. doi:10.1086/323920. ISSN 0004-6256.
- ^ Palmer, D. R.; Walker, E. N.; Jones, D. H. P.; Wallis, R. E. (1968). "The radial velocities spectral types and projected rotational velocities of 633 bright northern A stars". Royal Greenwich Observatory Bulletins. 135: 385. Bibcode:1968RGOB..135..385P.
- ^ Abt, Helmut A.; Morrell, Nidia I. (July 1995). "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars". The Astrophysical Journal Supplement Series. 99: 135. Bibcode:1995ApJS...99..135A. doi:10.1086/192182. ISSN 0067-0049.
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