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HR 1170

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Variable star in the constellation Perseus
HR 1170
Location of HR 1170 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Perseus
Right ascension 03 49 08.10977
Declination +43° 57′ 47.3016″
Apparent magnitude (V) 5.77 - 5.91
Characteristics
Spectral type A9IV
U−B color index 0.06
B−V color index 0.26
Variable type Delta Scuti
Astrometry
Radial velocity (Rv)−11.1±2.6 km/s
Proper motion (μ) RA: −3.453±0.244 mas/yr
Dec.: 11.469±0.200 mas/yr
Parallax (π)14.6959 ± 0.2134 mas
Distance222 ± 3 ly
(68.0 ± 1.0 pc)
Absolute magnitude (MV)1.73±0.07
Details
Mass1.98±0.04 M
Radius2.7 R
Luminosity23±2 L
Surface gravity (log g)3.77 cgs
Temperature7194±50 K
Metallicity 0.30 dex
Rotational velocity (v sin i)103 km/s
Age1.12 Gyr
Other designations
V376 Per, HD 23728, HIP 17846, SAO 39128
Database references
SIMBADdata

HR 1170, also known as HD 23728 and V376 Persei, is a star about 220 light years from the Earth, in the constellation Perseus. It is a 5th magnitude star, so it will be faintly visible to the naked eye of an observer far from city lights. It is a variable star, whose brightness varies slightly from magnitude 5.77 to 5.91.

A light curve for V376 Persei, plotted from TESS data

Michel Breger announced that HR 1170 is a Delta Scuti variable star in 1969, based on observations taken over 6 hours and 10 minutes on October 13, 1967. He reported that it varied with a mean amplitude of 0.08 magnitudes, over a period of 2.2 hours. In 1970 it was given the variable star designation V376 Persei.

Early investigations of HR 1170 showed that it has more than one pulsation period, as is true for most Delta Scuti stars, and the light curve shows the different periods beating with each other. Many investigators have tried to determine the modes of oscillation present in this star. All but one of these studies find only two significant periods. All agree that one of the periods is approximately 2.386 hours, but the studies do not agree on the second period. There is also no agreement as to whether the pulsations are radial, nonradial or a combination of the two, though most of the later studies, which examine data taken over a longer time window, conclude that at least one of the pulsation modes is nonradial.

References

  1. ^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  2. ^ Samus', N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
  3. ^ Netopil, Martin (August 2017). "Metallicity calibrations for dwarf stars and giants in the Geneva photometric system". Monthly Notices of the Royal Astronomical Society. 469 (3): 3042–3055. arXiv:1705.00883. Bibcode:2017MNRAS.469.3042N. doi:10.1093/mnras/stx1077. Retrieved 12 March 2023.
  4. ^ Oja, T. (August 1991). "UBV photometry of stars whose positions are accurately known. VI". Astronomy and Astrophysics Supplement Series. 89: 415–419. Bibcode:1991A&AS...89..415O. Retrieved 14 March 2023.
  5. 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. Retrieved 12 March 2023.
  6. Barac, Natascha; Bedding, Timothy R.; Murphy, Simon J.; Hey, Daniel R. (October 2022). "Revisiting bright δ Scuti stars and their period-luminosity relation with TESS and Gaia DR3". Monthly Notices of the Royal Astronomical Society. 516 (2): 2080–2094. arXiv:2207.00343. Bibcode:2022MNRAS.516.2080B. doi:10.1093/mnras/stac2132. Retrieved 12 March 2023.
  7. ^ 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. Retrieved 12 March 2023.
  8. Soubiran, C.; Le Campion, J. F.; Cayrel de Strobel, G.; Caillo, A. (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. Retrieved 12 March 2023.
  9. "HD 151804 -- Blue Supergiant". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2023-03-03.
  10. "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 11 March 2023.
  11. Breger, M. (March 1969). "Short-period variability of B, A, and F stars. II. Photometry of new Delta Scuti stars". Astronomical Journal. 74: 166–176. Bibcode:1969AJ.....74..166B. doi:10.1086/110788.
  12. Kukarkin, B. V.; Kholopov, P. N.; Perova, N. B. (October 1970). "57th Name-List of Variable Stars". Information Bulletin on Variable Stars. 480: 1. Bibcode:1970IBVS..480....1K. Retrieved 12 March 2023.
  13. Warman, J.; Malacara, Z.; Breger, M. (November 1974). "The light curves of Delta Scuti stars HR 1170 and HR 7563". Revista Mexicana de Astronomía y Astrofísica. 1: 143–150. Bibcode:1974RMxAA...1..143W. Retrieved 14 March 2023.
  14. Jayasinghe, T.; Stanek, K. Z.; Kochanek, C. S.; Vallely, P. J.; Shappee, B. J.; Holoien, T. W. S.; Thompson, Todd A.; Prieto, J. L.; Pejcha, O.; Fausnaugh, M.; Otero, S.; Hurst, N.; Will, D. (April 2020). "The ASAS-SN catalogue of variable stars VI: an all-sky sample of δ Scuti stars". Monthly Notices of the Royal Astronomical Society. 493 (3): 4186–4208. arXiv:1910.14187. Bibcode:2020MNRAS.493.4186J. doi:10.1093/mnras/staa499. Retrieved 14 March 2023.
  15. Breger, M.; Bregman, J. N. (September 1975). "Period-luminosity-color relations and pulsation modes of pulsating variable stars". Astrophysical Journal. 200: 343–353. Bibcode:1975ApJ...200..343B. doi:10.1086/153794.
  16. Gupta, S. K. (May 1977). "Study of the Delta Scuti Star HR 1170". Astrophysics and Space Science. 48 (1): 199–206. Bibcode:1977Ap&SS..48..199G. doi:10.1007/BF00643051. Retrieved 14 March 2023.
  17. Pena, J. H.; Warman, J. (July 1979). "HR 1170 and HR 7331, two nonradial Delta Scuti pulsators". Astronomical Journal. 84: 1046–1055. Bibcode:1979AJ.....84.1046P. doi:10.1086/112511. Retrieved 14 March 2023.
  18. Pena, J. H.; Warman, J. (April 1980). "On the periods of the del SCT star HR 1170". Revista Mexicana de Astronomía y Astrofísica. 5: 5–7. Bibcode:1980RMxAA...5....5P. Retrieved 14 March 2023.
  19. ^ Warman, J.; Pena, J. H.; Margrave, T. E. (October 1980). "Nonradial period structure of the del SCT star HR 1170". Publications of the Astronomical Society of the Pacific. 92: 696–699. Bibcode:1980PASP...92..696W. doi:10.1086/130732.
  20. Kurtz, D. W. (March 1981). "Radial and non-radial oscillations in the Del SCT star HR 1170". Monthly Notices of the Royal Astronomical Society. 194: 747–754. Bibcode:1981MNRAS.194..747K. doi:10.1093/mnras/194.3.747. Retrieved 14 March 2023.
  21. ^ Ostermann, W. M. (February 1990). "Pulsation periods in theδ Scuti star HR 1170". Astrophysics and Space Science. 164 (1): 87–93. Bibcode:1990Ap&SS.164...87O. doi:10.1007/BF00653553. Retrieved 14 March 2023.
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