Articles with "mass stars" as a keyword



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ALMA observations of RCW 120 Fragmentation at 0.01 pc scale

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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… read more here.

Keywords: mass stars; mass; rcw 120; fragmentation ... See more keywords
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Low Mass Stars as Tracers of Star and Cluster Formation

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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… read more here.

Keywords: formation; mass stars; low mass; molecular clouds ... See more keywords
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The accretion history of high-mass stars: an ArTéMiS pilot study of infrared dark clouds

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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… read more here.

Keywords: mass stars; accretion history; high mass; mass ... See more keywords
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Mirror principle and the red-giant bump: the battle of entropy in low-mass stars

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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… read more here.

Keywords: mass stars; luminosity; red giant; low mass ... See more keywords
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Fragmentation favoured in discs around higher mass stars

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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… read more here.

Keywords: mass stars; mass; higher mass; fragmentation ... See more keywords
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Massive discs around low-mass stars

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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… read more here.

Keywords: mass stars; mass; self gravity; low mass ... See more keywords