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Published in 2018 at "Astronomy and Astrophysics"
DOI: 10.1051/0004-6361/201832930
Abstract: Context. Little is known about how high-mass stars form. Around 30% of the young high-mass stars in the Galaxy are observed at the edges of ionized (H ii) regions. Therefore these are places of choice…
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Keywords:
mass stars;
mass;
rcw 120;
fragmentation ... See more keywords
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Published in 2022 at "Publications of the Astronomical Society of the Pacific"
DOI: 10.1088/1538-3873/ac4c9c
Abstract: We review the use of young low mass stars and protostars, or young stellar objects (YSOs), as tracers of star formation. Observations of molecular clouds at visible, infrared, radio and X-ray wavelengths can identify and…
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Keywords:
formation;
mass stars;
low mass;
molecular clouds ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1656
Abstract: The mass growth of protostars is a central element to the determination of fundamental stellar population properties such as the initial mass function. Constraining the accretion history of individual protostars is therefore an important aspect…
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Keywords:
mass stars;
accretion history;
high mass;
mass ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa176
Abstract: The evolution of low-mass stars into red giants is still poorly understood. During this evolution the core of the star contracts and, simultaneously, the envelope expands -- a process known as the `mirror'. Additionally, there…
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Keywords:
mass stars;
luminosity;
red giant;
low mass ... See more keywords
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1
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/staa883
Abstract: We use a suite of SPH simulations to investigate the susceptibility of protoplanetary discs to the effects of self-gravity as a function of star-disc properties. We also include passive irradiation from the host star using…
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Keywords:
mass stars;
mass;
self gravity;
low mass ... See more keywords