JWST and ALMA data provide the earliest direct evidence of ram-pressure stripping in a post-starburst galaxy at z=3.06, implying the process can quench star formation in nascent groups at z>3.
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R., Indebetouw, R., Brogan, C
11 Pith papers cite this work, alongside 68 external citations. Polarity classification is still indexing.
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First large-scale ACA CO(1-0) map of Stephan's Quintet identifies molecular gas structures and a negative SFE-velocity dispersion correlation, implying turbulence regulates star formation in this interacting group.
Serendipitous discovery of a bound nine-member protostellar system in NGC 6334-43 formed by filament fragmentation, with outflows from two sources and virial masses derived for three cores.
ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
Kpc-resolution ALMA CO and dust maps of three z~3 dusty galaxies are consistent with gravo-turbulent star-formation models rather than non-turbulent predictions.
Detection of 13-day variability at 100 GHz suggests a Compton-thick AGN in the Antennae galaxies.
Observational study of 100 LMC GMCs finds median 13CO(2-1)/12CO(2-1) line ratio of 0.078, nearly linear with luminosity, and higher in clouds hosting IR-bright young stellar objects.
ALMA observations of five DSFGs in the Spiderweb protocluster reveal disturbed molecular gas kinematics, field-like gas fractions that are lower in massive/AGN hosts, and declining gas content and sSFR with proximity to the central galaxy.
A GPU-accelerated Python software correlator enables real-time FX correlation, RFI flagging, calibration, and synthesis imaging for a four-antenna radio array on QUEST.
The paper proposes the iSEEDs project to integrate machine learning with astrochemistry for extracting physical conditions and molecular abundances from protostellar disk datasets.
Involving general users in prioritizing development for scientific software like CASA improves alignment with user needs and benefits both communities despite limited support resources.
citing papers explorer
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A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06
JWST and ALMA data provide the earliest direct evidence of ram-pressure stripping in a post-starburst galaxy at z=3.06, implying the process can quench star formation in nascent groups at z>3.
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Molecular Gas Structure and Star Formation Diversity in Stephan's Quintet Revealed by ACA CO(1-0) Mapping
First large-scale ACA CO(1-0) map of Stephan's Quintet identifies molecular gas structures and a negative SFE-velocity dispersion correlation, implying turbulence regulates star formation in this interacting group.
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A nine-member protostellar system forming via filament fragmentation in the high mass protocluster NGC 6334-43
Serendipitous discovery of a bound nine-member protostellar system in NGC 6334-43 formed by filament fragmentation, with outflows from two sources and virial masses derived for three cores.
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The Radial and Vertical Structure of Molecular Gas in the Edge-On Galaxy NGC 4565
ALMA CO observations of NGC 4565 reveal a thin non-flaring molecular disk with a central gap, consistent GMC properties to 17 kpc, and a prominent star-forming ring feature.
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Investigating the role of turbulence in the interstellar medium in $z\sim3$ dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps
Kpc-resolution ALMA CO and dust maps of three z~3 dusty galaxies are consistent with gravo-turbulent star-formation models rather than non-turbulent predictions.
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An AGN in the Antennae galaxies ?
Detection of 13-day variability at 100 GHz suggests a Compton-thick AGN in the Antennae galaxies.
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The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud
Observational study of 100 LMC GMCs finds median 13CO(2-1)/12CO(2-1) line ratio of 0.078, nearly linear with luminosity, and higher in clouds hosting IR-bright young stellar objects.
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Chaotic Molecular Gas in Five Dusty Star-forming Galaxies in the Spiderweb Protocluster at $z = 2.16$
ALMA observations of five DSFGs in the Spiderweb protocluster reveal disturbed molecular gas kinematics, field-like gas fractions that are lower in massive/AGN hosts, and declining gas content and sSFR with proximity to the central galaxy.
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A Python/CuPy Software Correlator for QUEST: Real-Time Performance and Initial Imaging
A GPU-accelerated Python software correlator enables real-time FX correlation, RFI flagging, calibration, and synthesis imaging for a four-antenna radio array on QUEST.
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Astrochemical Study of Early Embedded Disks
The paper proposes the iSEEDs project to integrate machine learning with astrochemistry for extracting physical conditions and molecular abundances from protostellar disk datasets.
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Role of General Users in the Lifecycle of Scientific Software
Involving general users in prioritizing development for scientific software like CASA improves alignment with user needs and benefits both communities despite limited support resources.