Search Results - "Monteiro, M. J. P. F. G."
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A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology
Published in Monthly notices of the Royal Astronomical Society (21-06-2011)“…The stratification near the base of the Sun's convective envelope is governed by processes of convective overshooting and element diffusion, and the region is…”
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Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission
Published in Science (American Association for the Advancement of Science) (08-04-2011)“…In addition to its search for extrasolar planets, the NASA Kepler mission provides exquisite data on stellar oscillations. We report the detections of…”
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Hybrid gamma Doradus-delta Scuti Pulsators: New Insights into the Physics of the Oscillations from Kepler Observations
Published 20-04-2010“…Observations of the pulsations of stars can be used to infer their interior structure and test theoretical models. The main-sequence γ Doradus (Dor) and δ…”
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Tests of parametric models for convection
Published in EPJ Web of Conferences (01-01-2015)“…In this study, we compare the effect of a modified convection parametrization in solar models on oscillation frequencies with different empirical correction…”
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Patterns, an efficient way to analyse the p-mode content in rapidly rotating stars
Published in EPJ Web of Conferences (01-01-2015)“…High precision photometric observations from space has led to the detection of hundreds of frequencies in the light curves of δ Scuti pulsators. In this work,…”
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The first view of δ Scuti and γ Doradus stars with the TESS mission
Published in Monthly notices of the Royal Astronomical Society (11-12-2019)“…ABSTRACT We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilize the 2-min…”
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Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods
Published in Monthly notices of the Royal Astronomical Society (11-07-2018)“…ABSTRACT Asteroseismic forward modelling techniques are being used to determine fundamental properties (e.g. mass, radius, and age) of solar-type stars. The…”
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Asteroseismic modelling of the Binary HD 176465
Published in EPJ Web of Conferences (01-01-2017)“…The detection and analysis of oscillations in binary star systems is critical in understanding stellar structure and evolution. This is partly because such…”
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Rotation and pulsation in Ap stars: first light results from TESS sectors 1 and 2
Published in Monthly notices of the Royal Astronomical Society (11-08-2019)“…Abstract We present the first results from the Transiting Exoplanet Survey Satellite (TESS) on the rotational and pulsational variability of magnetic…”
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TESTING SCALING RELATIONS FOR SOLAR-LIKE OSCILLATIONS FROM THE MAIN SEQUENCE TO RED GIANTS USING KEPLER DATA
Published in The Astrophysical journal (20-12-2011)“…We have analyzed solar-like oscillations in ~1700 stars observed by the Kepler Mission, spanning from the main sequence to the red clump. Using evolutionary…”
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PLATO hare-and-hounds exercise: asteroseismic model fitting of main-sequence solar-like pulsators
Published in Monthly notices of the Royal Astronomical Society (01-12-2021)“…ABSTRACT Asteroseismology is a powerful tool to infer fundamental stellar properties. The use of these asteroseismic-inferred properties in a growing number of…”
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FUNDAMENTAL PROPERTIES OF STARS USING ASTEROSEISMOLOGY FROM KEPLER AND CoRoT AND INTERFEROMETRY FROM THE CHARA ARRAY
Published in The Astrophysical journal (20-11-2012)“…We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five…”
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α Centauri A as a potential stellar model calibrator: establishing the nature of its core
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2018)“…ABSTRACT Understanding the physical process responsible for the transport of energy in the core of α Centauri A is of the utmost importance if this star is to…”
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MEASUREMENT OF ACOUSTIC GLITCHES IN SOLAR-TYPE STARS FROM OSCILLATION FREQUENCIES OBSERVED BY KEPLER
Published in The Astrophysical journal (10-02-2014)“…For the very best and brightest asteroseismic solar-type targets observed by Kepler, the frequency precision is sufficient to determine the acoustic depths of…”
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A Precise Asteroseismic Age and Radius for the Evolved Sun-like Star KIC 11026764
Published in The Astrophysical journal (10-11-2010)“…The primary science goal of the Kepler Mission is to provide a census of exoplanets in the solar neighborhood, including the identification and…”
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A large sample of calibration stars for Gaia: log g from Kepler and CoRoT fields
Published in Monthly notices of the Royal Astronomical Society (21-05-2013)“…Asteroseismic data can be used to determine stellar surface gravities with precisions of <0.05 dex by using the global seismic quantities 〈Δν〉 and νmax along…”
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Solar-like Oscillations in KIC 11395018 and KIC 11234888 from 8 Months of Kepler Data
Published in The Astrophysical journal (01-06-2011)“…We analyze the photometric short-cadence data obtained with the Kepler mission during the first 8 months of observations of two solar-type stars of spectral…”
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Atmospheric parameters and pulsational properties for a sample of δ Sct, γ Dor and hybrid Kepler targets
Published in Monthly notices of the Royal Astronomical Society (2011)“…We report spectroscopic observations for 19 δ Sct candidates observed by the Kepler satellite both in long and short cadence mode. For all these stars, by…”
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Asteroseismology and interferometry
Published in The Astronomy and astrophysics review (01-11-2007)“…Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the…”
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CHARACTERIZING TWO SOLAR-TYPE KEPLER SUBGIANTS WITH ASTEROSEISMOLOGY: KIC 10920273 AND KIC 11395018
Published in The Astrophysical journal (20-01-2013)“…Determining fundamental properties of stars through stellar modeling has improved substantially due to recent advances in asteroseismology. Thanks to the…”
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