| 词条 | Y Sextantis |
| 释义 |
| name = Y Sextantis }}{{Starbox image | image = | caption = Possible architecture for Y Sextantis' multiple system }}{{Starbox observe | epoch = J2000.0 | constell = Sextans | ra={{RA|10|02|47.9589}} | dec={{DEC|+01|05|40.346}} | appmag_v = 9.97 }}{{Starbox character | class = F8V/F8.5V-VI }}{{Starbox astrometry | dist_ly = 361.4 | dist_pc = 110.86 }}{{Starbox detail | mass = 1.21/0.22[1] | radius = 1.4/0.85 | luminosity = 2.6/0.96 | temperature = ≈6200 }}{{Starbox catalog | names = Y Sex, BD+01° 2394, HIP 49217, HD 87079 }}{{Starbox reference | Simbad = Y+Sex }}{{Starbox end}} Y Sextantis (abbreviated as Y Sex) is a W Ursae Majoris variable eclipsing contact binary star system located roughly at 360 light years from the Sun, whose two component stars share a common outer layer. Because the two components share their outer layers as the components of W Ursae Majoris do, they have the same stellar classification, and are classified as yellow F-type main sequence dwarfs. The components take 0.419822800 days (roughly 10 hours) to revolve around common barycentre. Orbital period variations would suggest the presence of additional perturbing objects, one of them likely substellar. Perturbing third (and fourth?) bodyOrbital period variations suggest the presence of one more perturbing unseen object.[1] The authors He & Qian have estimated two possible orbital periods and minimum masses for unseen companions: the former cyclic oscillation would occur every 51.22 years (with amplitude of 0.0218 days) being caused by a low-mass stellar companion (likely a M dwarf star), whereas the latter would consist in a 32.1 years period and the unseen object could likely be substellar. {{OrbitboxPlanet begin}}{{OrbitboxPlanet hypothetical| exoplanet = C | mass = ≥240 (0.24 Solar masses) | period = ≈18695 | semimajor = 49.0±3.9 | eccentricity = ? }}{{OrbitboxPlanet hypothetical | exoplanet = b | mass = ≥43 | period = ≈11716 | semimajor = 58.9±6.7 | eccentricity = ? }}{{Orbitbox end}} References1. ^1 {{cite journal | arxiv=0908.4521| author=He| author2=Qian| last-author-amp=yes | title=An Orbital Period Investigation of the WUMa-Type Binary Y Sextantis| journal=Publications of the Astronomical Society of Japan| volume=59| issue=6| pages=1115–1119| date=2007| bibcode=2007PASJ...59.1115H| doi=10.1093/pasj/59.6.1115}} {{Stars of Sextans}} 7 : Sextans (constellation)|Objects with variable star designations|F-type main-sequence stars|W Ursae Majoris variables|Hipparcos objects|Henry Draper Catalogue objects|Durchmusterung objects |
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