Search Results - "Montalbán, Josefina"
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HAYDN
Published in Experimental astronomy (01-06-2021)“…In the last decade, the Kepler and CoRoT space-photometry missions have demonstrated the potential of asteroseismology as a novel, versatile and powerful tool…”
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Determining stellar parameters of asteroseismic targets: going beyond the use of scaling relations
Published in Monthly notices of the Royal Astronomical Society (17-01-2017)“…Abstract Asteroseismic parameters allow us to measure the basic stellar properties of field giants observed far across the Galaxy. Most of such determinations…”
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A NEW GENERATION OF PARSEC-COLIBRI STELLAR ISOCHRONES INCLUDING THE TP-AGB PHASE
Published in The Astrophysical journal (20-01-2017)“…We introduce a new generation of PARSEC-COLIBRI stellar isochrones that includes a detailed treatment of the thermally pulsing asymptotic giant branch (TP-AGB)…”
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A New Interpretation of the Period-Luminosity Sequences of Long-period Variables
Published in The Astrophysical journal (01-10-2017)“…Period-luminosity (PL) sequences of long-period variables (LPVs) are commonly interpreted as different pulsation modes, but there is disagreement on the modal…”
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Modelling long-period variables – I. A new grid of O-rich and C-rich pulsation models
Published in Monthly notices of the Royal Astronomical Society (01-01-2019)Get full text
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Chronologically dating the early assembly of the Milky Way
Published in Nature astronomy (01-07-2021)“…The standard cosmological model predicts that galaxies are built through hierarchical assembly on cosmological timescales 1 , 2 . The Milky Way, like other…”
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Uncertainties on near-core mixing in red-clump stars: effects on the period spacing and on the luminosity of the AGB bump
Published in Monthly notices of the Royal Astronomical Society (01-11-2015)“…Low-mass stars in the He-core-burning (HeCB) phase play a major role in stellar, galactic, and extragalactic astrophysics. The ability to predict accurately…”
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Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Small Magellanic Cloud
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…Abstract The thermally pulsing asymptotic giant branch (TP-AGB) experienced by low- and intermediate-mass stars is one of the most uncertain phases of stellar…”
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Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars
Published in Nature (London) (31-03-2011)“…Kepler-based asteroseismology sorts red giants NASA's Kepler mission has been remarkably productive in its primary role, that of discovering and characterizing…”
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The Red-giant Branch Bump Revisited: Constraints on Envelope Overshooting in a Wide Range of Masses and Metallicities
Published in The Astrophysical journal (01-06-2018)“…The red-giant branch bump provides valuable information for the investigation of the internal structure of low-mass stars. Because current models are unable to…”
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Probing the properties of convective cores through g modes: high-order g modes in SPB and γ Doradus stars
Published in Monthly notices of the Royal Astronomical Society (2008)“…In main-sequence stars, the periods of high-order gravity modes are sensitive probes of stellar cores and, in particular, of the chemical composition gradient…”
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Bayesian distances and extinctions for giants observed by Kepler and APOGEE
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)“…We present a first determination of distances and extinctions for individual stars in the first release of the APOKASC catalogue, built from the joint efforts…”
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Deviations from a uniform period spacing of gravity modes in a massive star
Published in Nature (London) (11-03-2010)“…The life of a star is dominantly determined by the physical processes in the stellar interior. Unfortunately, we still have a poor understanding of how the…”
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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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Investigating surface correction relations for RGB stars
Published in Monthly notices of the Royal Astronomical Society (11-07-2020)“…ABSTRACT State-of-the-art stellar structure and evolution codes fail to adequately describe turbulent convection. For stars with convective envelopes such as…”
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Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes
Published in Nature (London) (05-01-2012)“…The core values of red giant stars The core rotation rate of a star, a key indicator of its evolutionary state, cannot be measured directly because the core is…”
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On the impact of the structural surface effect on global stellar properties and asteroseismic analyses
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT In a series of papers, we have recently demonstrated that it is possible to construct stellar structure models that robustly mimic the stratification…”
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HAYDN: High-precision AsteroseismologY of DeNse stellar fields
Published in Experimental astronomy (01-06-2021)“…In the last decade, the Kepler and CoRoT space-photometry missions have demonstrated the potential of asteroseismology as a novel, versatile and powerful tool…”
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Journal Article Web Resource