| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lyra |
| Right ascension | 19h 11m 46.008s [2] |
| Declination | +31° 17′ 00.44″ [2] |
| Apparent magnitude (V) | 5.93 [3] |
| Characteristics | |
| Spectral type | B8 IIIp Si Sr [4] |
| B−V color index | −0.062±0.004 [3] |
| Variable type | α2 CVn [5] |
| Astrometry | |
| Radial velocity (Rv) | −30.1±2.9 [3] km/s |
| Proper motion (μ) |
RA: −4.143
mas/
yr
[2] Dec.: −2.763 mas/ yr [2] |
| Parallax (π) | 3.4213 ± 0.0417 mas [2] |
| Distance | 950 ± 10
ly (292 ± 4 pc) |
| Absolute magnitude (MV) | −1.24 [3] |
| Details | |
| Mass | 3.76±0.22 [6] M☉ |
| Radius | 6.40 [7] R☉ |
| Luminosity | 397.48 [3] L☉ |
| Temperature | 11,194+501 −479 [6] K |
| Rotational velocity (v sin i) | 35 [8] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
19 Lyrae is a single [10] variable star located approximately 950 [2] light years away from the Sun in the northern constellation of Lyra. [9] It has the variable star designation V471 Lyr, while 19 Lyrae is the Flamsteed designation. This object is just bright enough to be visible to the naked eye, appearing as a dim, blue-white star with a baseline apparent visual magnitude of 5.93. [3] It is moving closer to the Earth with a heliocentric radial velocity of −30 km/s, and may come as close as 167 light-years around 8.5 million years from now. [3]
This is a magnetic chemically-peculiar star [11] with a stellar classification of B8 IIIp Si Sr, [4] showing abundance anomalies in silicon and strontium. The light variations of this star were discovered by J. E. Winzer in 1974. [12] It is an Alpha2 Canum Venaticorum-type variable with a period of 1.160898 days (or 7.0980 days [12]), ranging in magnitude from a high of 5.91 down to 5.98. [5] The surface magnetic field has a strength of (111.3±56.9)×10−4 T [13]
19 Lyrae has a moderate rotation rate, showing a projected rotational velocity of 35 km/s. [8] Stellar models give it an estimated 3.8 [6] times the mass of the Sun and its girth is measured at 6.4 [7] times the Sun's radius. It is radiating 397 [3] times the luminosity of the Sun from its photosphere at an effective temperature of around 11,194 K. [6] The star has an absolute magnitude of −1.24, [3] which shows how bright the star would appear if it were located at a distance of 10 parsecs (33 ly) from the Sun.
References
- ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved 8 December 2021.
- ^ a b c d e 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 f g h i 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 Abt, Helmut A.; Morrell, Nidia I. (1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars", Astrophysical Journal Supplement, 99: 135, Bibcode: 1995ApJS...99..135A, doi: 10.1086/192182
- ^ a b Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/s1063772917010085, S2CID 125853869.
- ^ a b c d Netopil, Martin; et al. (July 2017), "An Investigation of the Rotational Properties of Magnetic Chemically Peculiar Stars", Monthly Notices of the Royal Astronomical Society, 468 (3): 2745–2756, arXiv: 1703.05218, Bibcode: 2017MNRAS.468.2745N, doi: 10.1093/mnras/stx674.
- ^ a b Shulyak, D.; et al. (2014), "Interferometry of chemically peculiar stars: Theoretical predictions versus modern observing facilities", Monthly Notices of the Royal Astronomical Society, 443 (2): 1629, arXiv: 1406.6093, Bibcode: 2014MNRAS.443.1629S, doi: 10.1093/mnras/stu1259.
- ^ a b Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590
- ^ a b "19 Lyr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-05-30.
- ^ 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.
- ^ Kochukhov, O.; Bagnulo, S. (2006), "Evolutionary state of magnetic chemically peculiar stars", Astronomy and Astrophysics, 450 (2): 763, arXiv: astro-ph/0601461, Bibcode: 2006A&A...450..763K, doi: 10.1051/0004-6361:20054596, S2CID 18596834
- ^ a b Adelman, S. J.; Rice, R. H. (April 1999), "UVBY photometry of the mCP stars HD 35298, 19 Lyrae, HD 192678, and HR 8216", Astronomy and Astrophysics Supplement, 136: 111–115, Bibcode: 1999A&AS..136..111A, doi: 10.1051/aas:1999202.
- ^ Bychkov, V. D.; et al. (2009), "Catalogue of averaged stellar effective magnetic fields - II. Re-discussion of chemically peculiar A and B stars", Monthly Notices of the Royal Astronomical Society, 394 (3): 1338, Bibcode: 2009MNRAS.394.1338B, doi: 10.1111/j.1365-2966.2008.14227.x, S2CID 120268049.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Lyra |
| Right ascension | 19h 11m 46.008s [2] |
| Declination | +31° 17′ 00.44″ [2] |
| Apparent magnitude (V) | 5.93 [3] |
| Characteristics | |
| Spectral type | B8 IIIp Si Sr [4] |
| B−V color index | −0.062±0.004 [3] |
| Variable type | α2 CVn [5] |
| Astrometry | |
| Radial velocity (Rv) | −30.1±2.9 [3] km/s |
| Proper motion (μ) |
RA: −4.143
mas/
yr
[2] Dec.: −2.763 mas/ yr [2] |
| Parallax (π) | 3.4213 ± 0.0417 mas [2] |
| Distance | 950 ± 10
ly (292 ± 4 pc) |
| Absolute magnitude (MV) | −1.24 [3] |
| Details | |
| Mass | 3.76±0.22 [6] M☉ |
| Radius | 6.40 [7] R☉ |
| Luminosity | 397.48 [3] L☉ |
| Temperature | 11,194+501 −479 [6] K |
| Rotational velocity (v sin i) | 35 [8] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
19 Lyrae is a single [10] variable star located approximately 950 [2] light years away from the Sun in the northern constellation of Lyra. [9] It has the variable star designation V471 Lyr, while 19 Lyrae is the Flamsteed designation. This object is just bright enough to be visible to the naked eye, appearing as a dim, blue-white star with a baseline apparent visual magnitude of 5.93. [3] It is moving closer to the Earth with a heliocentric radial velocity of −30 km/s, and may come as close as 167 light-years around 8.5 million years from now. [3]
This is a magnetic chemically-peculiar star [11] with a stellar classification of B8 IIIp Si Sr, [4] showing abundance anomalies in silicon and strontium. The light variations of this star were discovered by J. E. Winzer in 1974. [12] It is an Alpha2 Canum Venaticorum-type variable with a period of 1.160898 days (or 7.0980 days [12]), ranging in magnitude from a high of 5.91 down to 5.98. [5] The surface magnetic field has a strength of (111.3±56.9)×10−4 T [13]
19 Lyrae has a moderate rotation rate, showing a projected rotational velocity of 35 km/s. [8] Stellar models give it an estimated 3.8 [6] times the mass of the Sun and its girth is measured at 6.4 [7] times the Sun's radius. It is radiating 397 [3] times the luminosity of the Sun from its photosphere at an effective temperature of around 11,194 K. [6] The star has an absolute magnitude of −1.24, [3] which shows how bright the star would appear if it were located at a distance of 10 parsecs (33 ly) from the Sun.
References
- ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, retrieved 8 December 2021.
- ^ a b c d e 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 f g h i 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 Abt, Helmut A.; Morrell, Nidia I. (1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars", Astrophysical Journal Supplement, 99: 135, Bibcode: 1995ApJS...99..135A, doi: 10.1086/192182
- ^ a b Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode: 2017ARep...61...80S, doi: 10.1134/s1063772917010085, S2CID 125853869.
- ^ a b c d Netopil, Martin; et al. (July 2017), "An Investigation of the Rotational Properties of Magnetic Chemically Peculiar Stars", Monthly Notices of the Royal Astronomical Society, 468 (3): 2745–2756, arXiv: 1703.05218, Bibcode: 2017MNRAS.468.2745N, doi: 10.1093/mnras/stx674.
- ^ a b Shulyak, D.; et al. (2014), "Interferometry of chemically peculiar stars: Theoretical predictions versus modern observing facilities", Monthly Notices of the Royal Astronomical Society, 443 (2): 1629, arXiv: 1406.6093, Bibcode: 2014MNRAS.443.1629S, doi: 10.1093/mnras/stu1259.
- ^ a b Abt, Helmut A.; et al. (July 2002), "Rotational Velocities of B Stars", The Astrophysical Journal, 573 (1): 359–365, Bibcode: 2002ApJ...573..359A, doi: 10.1086/340590
- ^ a b "19 Lyr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-05-30.
- ^ 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.
- ^ Kochukhov, O.; Bagnulo, S. (2006), "Evolutionary state of magnetic chemically peculiar stars", Astronomy and Astrophysics, 450 (2): 763, arXiv: astro-ph/0601461, Bibcode: 2006A&A...450..763K, doi: 10.1051/0004-6361:20054596, S2CID 18596834
- ^ a b Adelman, S. J.; Rice, R. H. (April 1999), "UVBY photometry of the mCP stars HD 35298, 19 Lyrae, HD 192678, and HR 8216", Astronomy and Astrophysics Supplement, 136: 111–115, Bibcode: 1999A&AS..136..111A, doi: 10.1051/aas:1999202.
- ^ Bychkov, V. D.; et al. (2009), "Catalogue of averaged stellar effective magnetic fields - II. Re-discussion of chemically peculiar A and B stars", Monthly Notices of the Royal Astronomical Society, 394 (3): 1338, Bibcode: 2009MNRAS.394.1338B, doi: 10.1111/j.1365-2966.2008.14227.x, S2CID 120268049.