EVOLUCION Y NUCLEOSINTESIS ESTELAR
EVOLUCION Y NUCLEOSINTESIS EST
Max Planck Institute for Astrophysics
Garching bei München, AlemaniaPublicaciones en colaboración con investigadores/as de Max Planck Institute for Astrophysics (13)
2023
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JWST Low-resolution MIRI Spectral Observations of SN 2021aefx: High-density Burning in a Type Ia Supernova
Astrophysical Journal Letters, Vol. 945, Núm. 1
2021
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Asteroseismic modelling of solar-type stars: A deeper look at the treatment of initial helium abundance
Monthly Notices of the Royal Astronomical Society, Vol. 500, Núm. 1, pp. 54-65
2020
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Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite
Astrophysical Journal Letters, Vol. 889, Núm. 2
2019
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Mode classification in fast-rotating stars using a convolutional neural network: Model-based regular patterns in ' Scuti stars
Monthly Notices of the Royal Astronomical Society: Letters, Vol. 483, Núm. 1, pp. L28-L32
2016
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Gamma-ray emission from SN2014J near maximum optical light
Astronomy and Astrophysics, Vol. 588
2015
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GAMMA RAYS from TYPE Ia SUPERNOVA SN 2014J
Astrophysical Journal, Vol. 812, Núm. 1
2014
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Cobalt-56 γ 3-ray emission lines from the type Ia supernova 2014J
Nature, Vol. 512, Núm. 7515, pp. 406-408
2010
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A precise asteroseismic age and radius for the evolved sun-like star KIC 11026764
Astrophysical Journal, Vol. 723, Núm. 2, pp. 1583-1598
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Detection of solar-like oscillations from kepler photometry of the open cluster NGC 6819
Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2
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The asteroseismic potential of kepler: First results for solar-type stars
Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2
2009
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Radius determination of solar-type stars using asteroseismology: What to expect from the kepler mission
Astrophysical Journal, Vol. 700, Núm. 2, pp. 1589-1602
2002
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Galactic evolution of 7LI: Observational clues for models
Astrophysics and Space Science
1997
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The cooling of co white dwarfs: Influence of the internal chemical distribution
Astrophysical Journal, Vol. 486, Núm. 1 PART I, pp. 413-419