Magnetic field properties in star formation: A review of their analysis methods and interpretation
J Liu, Q Zhang, K Qiu - Frontiers in Astronomy and Space Sciences, 2022 - frontiersin.org
Linearly polarized emission from dust grains and molecular spectroscopy is an effective
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …
probe of the magnetic field topology in the interstellar medium and molecular clouds. The …
Filament identification through mathematical morphology
EW Koch, EW Rosolowsky - Monthly Notices of the Royal …, 2015 - academic.oup.com
We present a new algorithm for detecting filamentary structure FilFinder. The algorithm uses
the techniques of mathematical morphology for filament identification, presenting a …
the techniques of mathematical morphology for filament identification, presenting a …
A uniform catalog of molecular clouds in the Milky Way
TS Rice, AA Goodman, EA Bergin… - The Astrophysical …, 2016 - iopscience.iop.org
The all-Galaxy CO survey of Dame et al. is by far the most uniform, large-scale Galactic CO
survey. Using a dendrogram-based decomposition of this survey, we present a catalog of …
survey. Using a dendrogram-based decomposition of this survey, we present a catalog of …
The green bank ammonia survey: First results of NH3 mapping of the gould belt
RK Friesen, JE Pineda, E Rosolowsky… - The Astrophysical …, 2017 - iopscience.iop.org
The Green Bank Ammonia Survey: First Results of NH3 Mapping of the Gould Belt - IOPscience
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This site uses cookies. By continuing to use this site you agree to our use of cookies. To find …
The VLA Nascent Disk and Multiplicity survey of Perseus protostars (VANDAM). V. 18 candidate disks around Class 0 and I protostars in the Perseus molecular cloud
DM Segura-Cox, LW Looney, JJ Tobin… - The Astrophysical …, 2018 - iopscience.iop.org
We present the full disk-fit results VANDAM survey of all Class 0 and I protostars in the
Perseus molecular cloud. We have 18 new protostellar disk candidates around Class 0 and I …
Perseus molecular cloud. We have 18 new protostellar disk candidates around Class 0 and I …
ALMA-IMF-XIII. N2H+ kinematic analysis of the intermediate protocluster G353. 41
RH Álvarez-Gutiérrez, AM Stutz… - Astronomy & …, 2024 - aanda.org
The ALMA-IMF Large Program provides multi-tracer observations of 15 Galactic massive
protoclusters at a matched sensitivity and spatial resolution. We focus on the dense gas …
protoclusters at a matched sensitivity and spatial resolution. We focus on the dense gas …
A cold accretion flow onto one component of a multiple protostellar system
NM Murillo, EF van Dishoeck, A Hacar… - Astronomy & …, 2022 - aanda.org
Context. Gas accretion flows transport material from the cloud core onto the protostar. In
multiple protostellar systems, it is not clear if the delivery mechanism is preferential or more …
multiple protostellar systems, it is not clear if the delivery mechanism is preferential or more …
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) survey of Perseus protostars. VI. Characterizing the formation mechanism for close multiple systems
Abstract We present Atacama Large Millimeter/submillimeter Array observations of multiple
protostar systems in the Perseus molecular cloud, previously detected by the Karl G. Jansky …
protostar systems in the Perseus molecular cloud, previously detected by the Karl G. Jansky …
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions–IX. A pilot study towards IRDC G034. 43+ 00.24 on multi-scale structures and gas …
We present a comprehensive study of the gas kinematics associated with density structures
at different spatial scales in the filamentary infrared dark cloud, G034. 43+ 00.24 (G34). This …
at different spatial scales in the filamentary infrared dark cloud, G034. 43+ 00.24 (G34). This …
The Davis–Chandrasekhar–Fermi method revisited
Despite the rich observational results on interstellar magnetic fields in star-forming regions, it
is still unclear how dynamically significant the magnetic fields are at varying physical scales …
is still unclear how dynamically significant the magnetic fields are at varying physical scales …