The molecular cloud lifecycle
M Chevance, JMD Kruijssen… - Space Science …, 2020 - Springer
Giant molecular clouds (GMCs) and their stellar offspring are the building blocks of galaxies.
The physical characteristics of GMCs and their evolution are tightly connected to galaxy …
The physical characteristics of GMCs and their evolution are tightly connected to galaxy …
Submillimeter and far-infrared polarimetric observations of magnetic fields in star-forming regions
K Pattle, L Fissel - Frontiers in Astronomy and Space Sciences, 2019 - frontiersin.org
Observations of star-forming regions by the current and upcoming generation of
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …
submillimeter polarimeters will shed new light on the evolution of magnetic fields over the …
The formation of massive molecular filaments and massive stars triggered by a magnetohydrodynamic shock wave
Recent observations suggest an that intensive molecular cloud collision can trigger massive
star/cluster formation. The most important physical process caused by the collision is a …
star/cluster formation. The most important physical process caused by the collision is a …
PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
Determining the atomic and molecular content of the interstellar medium (ISM) is of
fundamental importance to understand the star-formation process. Although there exist …
fundamental importance to understand the star-formation process. Although there exist …
Photodissociation region diagnostics across galactic environments
We present three-dimensional astrochemical simulations and synthetic observations of
magnetized, turbulent, self-gravitating molecular clouds. We explore various galactic …
magnetized, turbulent, self-gravitating molecular clouds. We explore various galactic …
Cosmic Evolution of Gas and Star Formation
Cosmic Evolution of Gas and Star Formation - IOPscience This site uses cookies. By continuing
to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies …
to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies …
An ALMA View of Molecular Filaments in the Large Magellanic Cloud. I. The Formation of High-mass Stars and Pillars in the N159E-Papillon Nebula Triggered by a …
We present ALMA observations of CO isotopes and 1.3 mm continuum emission toward the
N159E-Papillon Nebula in the Large Magellanic Cloud (LMC). The spatial resolution is 0 25 …
N159E-Papillon Nebula in the Large Magellanic Cloud (LMC). The spatial resolution is 0 25 …
A holistic perspective on the dynamics of G035. 39-00.33: the interplay between gas and magnetic fields
T Liu, PS Li, M Juvela, KT Kim, NJ Evans II… - The Astrophysical …, 2018 - iopscience.iop.org
Magnetic field plays a crucial role in shaping molecular clouds and regulating star formation,
yet the complete information on the magnetic field is not well constrained owing to the …
yet the complete information on the magnetic field is not well constrained owing to the …
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
H Takemura, F Nakamura, HG Arce… - The Astrophysical …, 2023 - iopscience.iop.org
The mass distribution of dense cores is a potential key to understanding the process of star
formation. Applying dendrogram analysis to the CARMA-NRO Orion C 18 O (J= 1–0) data …
formation. Applying dendrogram analysis to the CARMA-NRO Orion C 18 O (J= 1–0) data …
Gmc collisions as triggers of star formation. iii. density and magnetically regulated star formation
We study giant molecular cloud (GMC) collisions and their ability to trigger star cluster
formation. We further develop our three-dimensional magnetized, turbulent, colliding GMC …
formation. We further develop our three-dimensional magnetized, turbulent, colliding GMC …