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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa187
Abstract: We investigate how a protoplanetary disc's susceptibility to gravitational instabilities and fragmentation depends on the mass of its host star. We use 1D disc models in conjunction with 3D SPH simulations to determine the critical…
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Keywords:
mass stars;
mass;
higher mass;
fragmentation ... See more keywords
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1
Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa2608
Abstract: Debris discs are second-generation dusty discs formed by collisions of planetesimals. Many debris discs have been found and resolved around hot and solar-type stars. However, only a handful have been discovered around M-stars, and the…
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Keywords:
around stars;
discs around;
debris discs;
discs ... See more keywords
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Published in 2021 at "Physical Review D"
DOI: 10.1103/physrevd.104.104055
Abstract: We study stable circular orbits (SCO) around static spherically symmetric configuration of General Relativity with a non-linear scalar field (SF). The configurations are described by solutions of the Einstein-SF equations with monomial SF potential V…
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Keywords:
spherically symmetric;
accretion;
discs around;
accretion discs ... See more keywords
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1
Published in 2018 at "Astronomy and Astrophysics"
DOI: 10.15496/publikation-30958
Abstract: We present high angular resolution (similar to 0.2 '') continuum and molecular emission line Atacama Large Millimeter/sub-millimeter Array (ALMA) observations of G17.64+0.16 in Band 6 (220-230 GHz) taken as part of a campaign in search…
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Keywords:
line;
proto stars;
discs around;
emission ... See more keywords