Publicación
Three element optical systems for efficient interferometry at sub-mm wavelengths.
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PublicaciónThree generations of stars: a possible case of triggered star formationEvidence for triggered star formation linking three generations of stars is difficult to assemble, as it requires convincingly associating evolved massive stars...
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PublicaciónThree hot Jupiters transiting K-dwarfs with significant heavy element massesContext. Despite predictions from planetary population synthesis models indicating that such systems should be exceedingly rare, short-period gas giants do...
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PublicaciónThree Long-period Transiting Giant Planets from TESSWe report the discovery and orbital characterization of three new transiting warm giant planets. These systems were initially identified as presenting single...
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PublicaciónThree Lyman-α-emitting filaments converging to a massive galaxy group at z = 2.91: discussing the case for cold gas infallWe have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive galaxy group RO-1001 at z = 2.91 in the Cosmic Evolution Survey field. Keck...
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PublicaciónThree new 2+2 quadruple systems with changing inclinationWe present a unique discovery of three new detected systems showing two different phenomena together. These are 2+2 quadruple stellar systems showing two...
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PublicaciónThree new young objects from the IRAS Point Source CatalogueThree new young objects have been found when carrying out a survey of IRAS sources with infrared colors like planetary nebulae, via low resolution spectroscopy...
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PublicaciónThree planets transiting the evolved star EPIC 249893012: a hot 8.8-M<SUB>⊕</SUB> super-Earth and two warm 14.7 and 10.2-M<SUB>⊕</SUB> sub-NeptunesWe report the discovery of a new planetary system with three transiting planets, one super-Earth and two sub-Neptunes, that orbit EPIC 249893012, a G8 IV-V...
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PublicaciónThree Red Giants With Substellar-Mass CompanionsWe present three giant stars from the ongoing Penn State–Toruń Planet Search with the Hobby–Eberly Telescope, which exhibit radial velocity (RV) variations that...