A Monopolar Jet from Protostar HOPS 10: Evidence for Asymmetric Magnetized Launching
A fundamental challenge in star formation is understanding how a protostar accretes mass from its circumstellar disk while removing excess angular momentum.
Somnath Dutta
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Molecular Jets from an Evolved Protostar: Insights from JWST-ALMA Synergy
The combination of the Atacama Large Millimeter/submillimeter Array (ALMA) and JWST/MIRI mid-infrared observations offers a transformative view of protostellar jets and outflows by probing cold and warm gas components across diverse physical conditions ...
Somnath Dutta
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We propose a new amorphous dust emission model based on the soft-potential (SP) model, applicable in the long-wavelength range from the far-infrared to the microwave.
Masashi Nashimoto
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The ALMA-ATOMS Survey: Exploring Protostellar Outflows in HC3N
We present the first systematic study of bipolar outflows using HC _3 N as a tracer in a sample of 146 massive star-forming regions from the Atacama Large Millimeter/submillimeter Array Three-millimeter Observations of Massive Star-forming Regions (ATOMS)
Ariful Hoque +27 more
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The ALMA survey of Gas Evolution in PROtoplanetary disks (AGE-PRO) Large Program aims to trace the evolution of gas disk mass and size throughout the lifetime of protoplanetary disks by using the Atacama Large Millimeter/submillimeter Array (ALMA).
Dary A. Ruiz-Rodriguez +19 more
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From Nobeyama Radio Observatory to the international project ALMA -Evolution of millimeter and submillimeter wave astronomy in Japan. [PDF]
Ishiguro M, Chiba K, Sakamoto S.
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RUBIES: JWST/NIRSpec Resolves Evolutionary Phases of Dusty Star-forming Galaxies at z ∼ 2
The dearth of high-quality spectroscopy of dusty star-forming galaxies (DSFGs)—the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe—greatly hinders our ability to interpret their physical processes and ...
Olivia R. Cooper +27 more
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High-dimensional Statistical Analysis and Its Application to an ALMA Map of NGC 253
In astronomy, if we denote the dimension of data as d and the number of samples as n , we often find a case with n ≪ d . Traditionally, such a situation is regarded as ill-posed, and there was no choice but to discard most of the information in data ...
Tsutomu T. Takeuchi +8 more
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First submillimeter lights from Dome A: Tracing the carbon cycle in the feedback of massive stars. [PDF]
Gong Y +40 more
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Candidate Sites for Millimeter and Submillimeter Ground-Based Telescopes: Atmospheric Rating for the Eurasian Submillimeter Telescopes Project. [PDF]
Shikhovtsev AY, Kovadlo PG, Baron P.
europepmc +1 more source

