prikaz prve stranice dokumenta Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri
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Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri
Astronomy and Astrophysics, 578 (2015); A25. https://doi.org/10.1051/0004-6361/201525873
Maxted, P. F. L.; Hutcheon, R. J.; Torres, G.; Lacy, C. H. S.; Southworth, J.; Smalley, B.; Pavlovski, Krešimir; Marchall, L. A.; Clausen, J. V.

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Maxted, P. F. L., Hutcheon, R. J., Torres, G., Lacy, C. H. S., Southworth, J., Smalley, B. ... Clausen, J. V. (2015). Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri. Astronomy and Astrophysics, 578.. doi: 10.1051/0004-6361/201525873

Maxted, P. F. L., et al. "Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri." Astronomy and Astrophysics, vol. 578, 2015. https://doi.org/10.1051/0004-6361/201525873

Maxted, P. F. L., R. J. Hutcheon, G. Torres, C. H. S. Lacy, J. Southworth, B. Smalley, Krešimir Pavlovski, L. A. Marchall i J. V. Clausen. "Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri." Astronomy and Astrophysics 578 (2015). https://doi.org/10.1051/0004-6361/201525873

Maxted, P. F. L., et al. (2015) 'Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri', Astronomy and Astrophysics, 578. doi: 10.1051/0004-6361/201525873

Maxted PFL, Hutcheon RJ, Torres G, Lacy CHS, Southworth J, Smalley B, i sur.. Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri. Astronomy and Astrophysics [Internet]. 2015. [pristupljeno 20.04.2024.];578. doi: 10.1051/0004-6361/201525873

P. F. L. Maxted, et al., "Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri", Astronomy and Astrophysics, vol. 578, 2015. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:434137. [Citirano: 20.04.2024.]

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Naslov (engleski)Precise mass and radius measurements for the components of the bright solar-type eclipsing binary star V1094 Tauri
AutorP. F. L. Maxted
AutorR. J. Hutcheon
AutorG. Torres
AutorC. H. S. Lacy
AutorJ. Southworth
AutorB. Smalley
AutorKrešimir Pavlovski
AutorL. A. Marchall
AutorJ. V. Clausen
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
Context. V1094 Tau is a bright eclipsing binary star with an orbital period close to nine days that contains two stars similar to the Sun. Aims. Our aim is to test models of Sun-like stars using precise and accurate mass and radius measurements for both stars in V1094 Tau. Methods. We present new spectroscopy of V1094 Tau, which we use to estimate the effective temperatures of both stars and to refine their spectroscopic orbits. We also present new, high-quality photometry covering both eclipses of V1094 Tau in the Strömgren uvby system and in the Johnson V-band. Results. The masses, radii, and effective temperatures of the stars in V1094 Tau are found to be M_A = 1.0965 ± 0.0040 M⊙, R_A = 1.4109 ± 0.0058 R⊙, T_eff, A = 5850 ± 100 K, M_B = 1.0120 ± 0.0028 M⊙, R_B = 1.1063 ± 0.0066 R⊙, and T_eff, B = 5700 ± 100 K. An analysis of the times of mid-eclipse and the radial velocity data reveals apsidal motion with a period of 14 500 ± 3700 years. Conclusions. The observed masses, radii, and effective temperatures are consistent with stellar models for an age ≈6 Gyr if the stars are assumed to have a metallicity similar to the Sun. This estimate is in reasonable agreement with our estimate of the metallicity derived using Strömgren photometry and treating the binary as a single star ([ Fe/H ] = −0.09 ± 0.11). The rotation velocities of the stars suggest that V1094 Tau is close to the limit at which tidal interactions between the stars force them to rotate pseudo-synchronously with the orbital motion.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstronomy and Astrophysics
Brojčani podacivol. 578, A25
p-ISSN0004-6361
DOIhttps://doi.org/10.1051/0004-6361/201525873
URN:NBNurn:nbn:hr:217:434137
Datum objave publikacije2015
URL dokumentahttps://www.aanda.org/articles/aa/abs/2015/06/aa25873-15/aa25873-15.html
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© ESO 2015. Received 11 February 2015. Accepted 15 March 2015. Published online 27 May 2015.
Datum i vrijeme pohrane2020-01-11 19:32:19