Martin Bo Nielsen researcher ORCID ID = 0000-0001-9169-2599
Bo Nielsen, Martin
VIAF ID: 135150565609106251408 (Personal)
Permalink: http://viaf.org/viaf/135150565609106251408
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Works
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Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi |
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Age determination of galaxy merger remnant stars using asteroseismology |
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Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7 |
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Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades |
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Butterfly diagram of a Sun-like star observed using asteroseismology |
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Differential rotation in Sun-like stars from surface variability and asteroseismology : doctoral thesis accepted by the University of Göttingen, Göttingen, Germany |
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Gaia16apd – a link between fast and slowly declining type I superluminous supernovae |
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Kepler observations of the asteroseismic binary HD 176465 |
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Latitudinal differential rotation in the solar analogues 16 Cygni A and B |
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Lifetimes and Rotation within the Solar Mean Magnetic Field |
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PBjam: A Python Package for Automating Asteroseismology of Solar-like Oscillators |
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The PLATO 2.0 mission |
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A probabilistic method for detecting solar-like oscillations using meaningful prior information |
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Rotation and magnetism of Kepler pulsating solar-like stars |
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Solar cycle variation of νmax in helioseismic data and its implications for asteroseismology |
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Sounding stellar cycles with Kepler – III. Comparative analysis of chromospheric, photometric, and asteroseismic variability |
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Spectroscopic classification of two supernova by NUTS (Nordic Optical Telescope Un-biased Transient Survey) |
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Starspot rotation rates versus activity cycle phase: Butterfly diagrams of Kepler stars are unlike that of the Sun |
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Starspot simulations forKepler |
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TESS asteroseismology of the known planet host star λ2 Fornacis |
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Testing the recovery of stellar rotation signals from Kepler light curves using a blind hare-and-hounds exercise |
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