Alpha Flying Fish ( α Volantis , α Vol ) is a double star [10] in the constellation Flying Fish . The apparent magnitude is +4.00, which is enough for observation with the naked eye. Based on the measurement of the annual parallax , an estimate of the distance from the Sun equal to 125 light years was obtained. As of 2010, the two components of the star system were separated by an angular distance of 0.0318 arc seconds at a position angle of 286.9 °. The magnitude difference of the two components is 0.1. [11] Perhaps he is a representative of the Sirius supercluster. [four]
| Alpha Flying Fish | |||
|---|---|---|---|
| Star | |||
| Observational data ( Age J2000.0 ) | |||
| Right ascension | |||
| Declination | |||
| Visible magnitude ( V ) | +4.00 [2] | ||
| Constellation | Flying fish | ||
| Astrometry | |||
| Radial velocity ( R v ) | +4.9 [3] km / s | ||
| Own movement (μ) | RA: −2.00 [1] Dec: +95.51 [1] | ||
| Parallax (π) | 26.11 ± 0.12 [1] mas | ||
| Absolute magnitude (V) | +1.60 [4] | ||
| Specifications | |||
| Spectral class | kA3hA5mA5 V [5] | ||
| Color Index ( B - V ) | +0.14 [2] | ||
| Color Index ( U - B ) | +0.13 [2] | ||
| physical characteristics | |||
| Weight | 1.87 [6] M ☉ | ||
| Radius | 1.9 [7] R ☉ | ||
| Age | 427 +183 −377 [8] Ma | ||
| Temperature | 8198 [5] K | ||
| Metallicity | +0.19 [5] | ||
| Rotation | 30.6 ± 0.4 [9] | ||
| |||
| Database Information | |||
| SIMBAD | data | ||
The main component is an Am star , the spectral class is kA3hA5mA5 V. [5] This notation shows that the star has a weak K line of ionized calcium as in class A3 stars, and hydrogen and metal lines like in a class A5 star. [12] Estimated age is 427 million years. [8] In 1992, it was discovered that the radiation of the star has an infrared excess , which indicates the presence of a circumstellar disk from dust. [13] However, subsequent observations have not confirmed the presence of the disc. [14]
Notes
- ↑ 1 2 3 4 5 van Leeuwen, F. (2007), " Validation of the new Hipparcos reduction ", Astronomy and Astrophysics T. 474 (2): 653–664 , DOI 10.1051 / 0004-6361: 20078357
- ↑ 1 2 3 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalog of Eggen's UBV data. SIMBAD
- ↑ Wielen, R .; Schwan, H .; Dettbarn, C. & Lenhardt, H. (1999), "Sixth Catalog of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions", Veröff. Astron. Rechen-Inst. Heidelb (Astronomisches Rechen-Institut Heidelberg). - T. 35 (35)
- ↑ 1 2 Eggen, Olin J. (August 1998), " The Sirius Supercluster and Missing Mass near the Sun, " The Astronomical Journal T. 116 (2): 782–788 , DOI 10.1086 / 300465
- ↑ 1 2 3 4 Gray, RO; Corbally, CJ; Garrison, RF & McFadden, MT (July 2006), " Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample ", The Astronomical Journal T. 132 (1): 161– 170 , DOI 10.1086 / 504637
- ↑ 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 T. 804 (2): 146 , DOI 10.1088 / 0004-637X / 804/2/146
- ↑ Pasinetti Fracassini, LE; Pastori, L .; Covino, S. & Pozzi, A. (February 2001), " Catalog of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition ", Astronomy and Astrophysics T. 367 (2): 521–524 , DOI 10.1051 / 0004 -6361: 20000451
- ↑ 1 2
- ↑ Díaz, CG; González, JF; Levato, H. & Grosso, M. (July 2011), " Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum ", Astronomy & Astrophysics T. 531: A143 , DOI 10.1051 / 0004-6361 / 201016386
- ↑ Eggleton, PP & Tokovinin, AA (September 2008), " A catalog of multiplicity among bright stellar systems ", Monthly Notices of the Royal Astronomical Society T. 389 (2): 869–879 , DOI 10.1111 / j.1365-2966.2008 .13596.x
- ↑ Hartkopf, William I .; Tokovinin, Andrei & Mason, Brian D. (2012), " Speckle Interferometry at SOAR in 2010 and 2011: Measures, Orbits, and Rectilinear Fits ", The Astronomical Journal T. 143 (2): 19, 42, doi : 10.1088 / 0004-6256 / 143/2/42 , < http://www.dtic.mil/get-tr-doc/pdf?AD=ADA556130 >
- ↑ Gray, Richard O. & Corbally, Christopher J. (2009), Stellar Spectral Classification , Princeton, New Jersey: Princeton University Press , p. 309, ISBN 978-0-691-12511-4
- ↑ Cheng, K.-P .; Bruhweiler, FC; Kondo, Y. & Grady, CA (September 1992), " Newly identified main-sequence A stars with circumstellar dust ", Astrophysical Journal, Part 2 T. 396 (2): L83 – L86 , DOI 10.1086 / 186522
- ↑ Gáspár, András; Rieke, George H. & Balog, Zoltán (May 2013), " The Collisional Evolution of Debris Disks ", The Astrophysical Journal T. 768 (1): 29, 25 , DOI 10.1088 / 0004-637X / 768/1/25