Search Results - "Aguirre, Victor Silva"
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The Fall of a Giant. Chemical evolution of Enceladus, alias the Gaia Sausage
Published in Monthly notices of the Royal Astronomical Society. Letters (01-07-2019)“…ABSTRACT We present the first chemical evolution model for Enceladus, alias the Gaia Sausage, to investigate the star formation history of one of the most…”
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Asteroseismic radii of dwarfs: new accuracy constraints from Gaia DR2 parallaxes
Published in Monthly notices of the Royal Astronomical Society. Letters (21-11-2018)“…Abstract Precise stellar masses and radii can be determined using asteroseismology, but their accuracy must be tested against independent estimates. Using…”
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Age-dating Red Giant Stars Associated with Galactic Disk and Halo Substructures
Published in The Astrophysical journal (01-08-2021)“…Abstract The vast majority of Milky Way stellar halo stars were likely accreted from a small number (≲3) of relatively large dwarf galaxy accretion events…”
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The K2 Galactic Archaeology Program Data Release 3: Age-abundance Patterns in C1–C8 and C10–C18
Published in The Astrophysical journal (01-02-2022)“…Abstract We present the third and final data release of the K2 Galactic Archaeology Program (K2 GAP) for Campaigns C1–C8 and C10–C18. We provide asteroseismic…”
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Stellar Spin-Orbit Misalignment in a Multiplanet System
Published in Science (American Association for the Advancement of Science) (18-10-2013)“…Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities…”
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Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the TESS continuous viewing zones and beyond
Published in Monthly notices of the Royal Astronomical Society (01-04-2021)“…ABSTRACT The NASA Transiting Exoplanet Survey Satellite (NASA-TESS) mission presents a treasure trove for understanding the stars it observes and the Milky…”
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Weighing stars from birth to death: mass determination methods across the HRD
Published in The Astronomy and astrophysics review (01-12-2021)“…The mass of a star is the most fundamental parameter for its structure, evolution, and final fate. It is particularly important for any kind of stellar…”
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TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion
Published in The Astrophysical journal (01-12-2021)“…Abstract Asteroseismology of bright stars has become increasingly important as a method to determine the fundamental properties (in particular ages) of stars…”
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A 20 Second Cadence View of Solar-type Stars and Their Planets with TESS: Asteroseismology of Solar Analogs and a Recharacterization of π Men c
Published in The Astronomical journal (01-02-2022)“…Abstract We present an analysis of the first 20 second cadence light curves obtained by the TESS space telescope during its extended mission. We find improved…”
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ACCURATE PARAMETERS OF THE OLDEST KNOWN ROCKY-EXOPLANET HOSTING SYSTEM: KEPLER-10 REVISITED
Published in The Astrophysical journal (01-02-2014)“…Since the discovery of Kepler-10, the system has received considerable interest because it contains a small, rocky planet which orbits the star in less than a…”
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Updated BaSTI Stellar Evolution Models and Isochrones. II. α-enhanced Calculations
Published in The Astrophysical journal (01-02-2021)“…Abstract This is the second paper of a series devoted to presenting an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model and…”
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Helium settling in F stars: constraining turbulent mixing using observed helium glitch signature
Published in Monthly notices of the Royal Astronomical Society (21-10-2019)“…ABSTRACT Recent developments in asteroseismology – due to space-based missions such as CoRoT and Kepler – provide handles on those properties of stars that…”
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The Updated BaSTI Stellar Evolution Models and Isochrones. I. Solar-scaled Calculations
Published in The Astrophysical journal (01-04-2018)“…We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar model and isochrone library for a solar-scaled heavy element…”
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THE K2 M67 STUDY: REVISITING OLD FRIENDS WITH K2 REVEALS OSCILLATING RED GIANTS IN THE OPEN CLUSTER M67
Published in The Astrophysical journal (01-12-2016)“…ABSTRACT Observations of stellar clusters have had a tremendous impact in forming our understanding of stellar evolution. The open cluster M67 has a…”
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Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars
Published in Nature (London) (14-01-2016)“…The age of a young to middle-aged star can be determined from how quickly or slowly it rotates, but the relationship breaks down for old stars; models now show…”
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When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147
Published in The Astrophysical journal (01-12-2020)“…Recent measurements of rotation periods ( ) in the benchmark open clusters Praesepe (670 Myr), NGC 6811 (1 Gyr), and NGC 752 (1.4 Gyr) demonstrate that, after…”
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Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes
Published in The Astrophysical journal (01-08-2017)“…We present a comparison of parallaxes and radii from asteroseismology and Gaia DR1 (TGAS) for 2200 Kepler stars spanning from the main sequence to the…”
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THE K2 GALACTIC ARCHAEOLOGY PROGRAM DATA RELEASE I: ASTEROSEISMIC RESULTS FROM CAMPAIGN 1
Published in The Astrophysical journal (20-01-2017)“…NASA's K2 mission is observing tens of thousands of stars along the ecliptic, providing data suitable for large-scale asteroseismic analyses to inform galactic…”
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Helium abundance in a sample of cool stars: measurements from asteroseismology
Published in Monthly notices of the Royal Astronomical Society (11-03-2019)Get full text
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Theoretical oscillation frequencies for solar-type dwarfs from stellar models with 〈3D〉-atmospheres
Published in Monthly notices of the Royal Astronomical Society (11-12-2017)“…Abstract We present a new method for replacing the outermost layers of stellar models with interpolated atmospheres based on results from 3D simulations, in…”
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