The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey:
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …
Clump Fragmentation - IOPscience This site uses cookies. By continuing to use this site you …
The origin of massive stars: The inertial-inflow model
We address the problem of the origin of massive stars, namely the origin, path, and
timescale of the mass flows that create them. Based on extensive numerical simulations, we …
timescale of the mass flows that create them. Based on extensive numerical simulations, we …
Magnetic fields in star formation: from clouds to cores
In this chapter we review recent advances in understanding the roles that magnetic fields
play throughout the star formation process, gained through observations and simulations of …
play throughout the star formation process, gained through observations and simulations of …
Mother of dragons-A massive, quiescent core in the dragon cloud (IRDC G028. 37+ 00.07)
Context. Core accretion models of massive star formation require the existence of massive,
starless cores within molecular clouds. Yet, only a small number of candidates for such truly …
starless cores within molecular clouds. Yet, only a small number of candidates for such truly …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). IV. Star Formation Signatures in G023. 477
K Morii, P Sanhueza, F Nakamura… - The Astrophysical …, 2021 - iopscience.iop.org
With a mass of∼ 1000 M⊙ and a surface density of∼ 0.5 g cm− 2, G023. 477+ 0.114, also
known as IRDC 18310-4, is an infrared dark cloud (IRDC) that has the potential to form high …
known as IRDC 18310-4, is an infrared dark cloud (IRDC) that has the potential to form high …
An alma view of molecular filaments in the large magellanic cloud. ii. an early stage of high-mass star formation embedded at colliding clouds in n159w-south
We have conducted ALMA CO isotopes and 1.3 mm continuum observations toward
filamentary molecular clouds of the N159W-South region in the Large Magellanic Cloud with …
filamentary molecular clouds of the N159W-South region in the Large Magellanic Cloud with …
A Census of Outflow to Magnetic Field Orientations in Nearby Molecular Clouds
D Xu, SSR Offner, R Gutermuth… - The Astrophysical …, 2022 - iopscience.iop.org
We define a sample of 200 protostellar outflows showing blue-and redshifted CO emission
in the nearby molecular clouds Ophiuchus, Taurus, Perseus, and Orion, to investigate the …
in the nearby molecular clouds Ophiuchus, Taurus, Perseus, and Orion, to investigate the …
Deep diving off the 'Cosmic Cliffs': previously hidden outflows in NGC 3324 revealed by JWST
M Reiter, JA Morse, N Smith, TJ Haworth… - Monthly Notices of …, 2022 - academic.oup.com
We present a detailed analysis of the protostellar outflow activity in the massive star-forming
region NGC 3324, as revealed by new Early Release Observations (EROs) from the James …
region NGC 3324, as revealed by new Early Release Observations (EROs) from the James …
Evolution of the Angular Momentum of Molecular Cloud Cores Formed from Filament Fragmentation
Y Misugi, S Inutsuka, D Arzoumanian - The Astrophysical Journal, 2023 - iopscience.iop.org
The angular momentum of molecular cloud cores plays an important role in the process of
star formation. However, the time evolution of the angular momentum of molecular cloud …
star formation. However, the time evolution of the angular momentum of molecular cloud …
ALMA–IRDC: dense gas mass distribution from cloud to core scales
AT Barnes, JD Henshaw, F Fontani… - Monthly Notices of …, 2021 - academic.oup.com
Infrared dark clouds (IRDCs) are potential hosts of the elusive early phases of high mass
star formation (HMSF). Here, we conduct an in-depth analysis of the fragmentation …
star formation (HMSF). Here, we conduct an in-depth analysis of the fragmentation …