European ARC Newsletter
29 Nov 2024

Welcome to the European ALMA Regional Centre Newsletter!  

This monthly newsletter is a compilation of recent European ALMA Regional Centre news and announcements, showcasing an exciting ALMA science result by European colleagues. Every month, you can learn an interesting ALMA fact in "Did you know" and give your opinion about a particular ALMA matter in the "Poll of the month".

News and announcements Science highlight Poll of the month Did you know


European ARC News and Announcements


Update on the Wideband Sensitivity Upgrade

28 Nov 2024:

Numerous ALMA staff worldwide remain actively involved in the preparation of the ALMA Wideband Sensitivity Upgrade (WSU). Regarding the advancement of development projects within the ALMA regions, the Data Transmission System successfully completed its Preliminary Design Review in Japan in October. Additionally, the Conceptual Design Review and the System Requirement Review for the Total Power GPU Spectrometer were also passed in October.

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AI-Driven Imaging: ESO's Internal ALMA Development Study 'BRAIN' Completed!

28 Nov 2024:


The BRAIN study pioneers the application of artificial intelligence (AI) to ALMA data, redefining imaging processes. By addressing challenges like extended emission detection and computational efficiency, the study introduces cutting-edge tools - RESOLVE and DeepFocus - to improve imaging quality and speed.

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Towards ALMA 2040

28 Nov 2024:

Following the announcement from ESO about the start of the search for its next astronomical ground-based programme for the 2040s (https://next.eso.org/), the community is getting organised to prepare the science case for a potential facility in the 2040s ('ALMA 2040'), building upon the successes of the current ALMA Observatory. 

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Registration open for Spanish ALMA Days

01 Nov 2024:

Spanish ALMA days will take place on 18-20 February 2025 and will be hosted by the Instituto de Astrofisica de Canarias (IAC) in Tenerife, Spain.

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ALMA science highlight

Disruption of a massive molecular cloud by a supernova in the Galactic Centre 

Figures from the paper
Left panel: HNCO (4-3) peak intensity map from ACES towards the M0.8-0.2 Ring. The dotted white circles show the approximate extent of the ring-like structure. Right panel: Multi-wavelength view of part of the CMZ, showing the location of the M0.8-0.2 Ring, indicated by the dotted white circles.

The Central Molecular Zone (CMZ) is the most extreme environment in the Milky Way. Located in the inner few hundred parsecs of our galaxy, the CMZ exhibits turbulent motions, magnetic field strengths, gas densities, pressures, and temperatures orders of magnitude greater than those measured in our local solar neighbourhood. The gas dynamics within the CMZ are similarly extreme, with strong gravitational shear capable of stretching molecular clouds. The extreme nature of the CMZ makes it the perfect laboratory to test theories of star formation in environments that differ from our galactic disc. The ALMA Central Molecular Zone Exploration Survey (ACES) provides an unprecedented, high-resolution view of the gas at the centre of our galaxy, seeking to better our understanding of this highly complex region.

Nonhebel et. al (2024) presents some of the first results from the ACES collaboration, exploring the morphology and kinematics of a ring-shaped molecular cloud with the CMZ. The M0.8-0.2 Ring is a highly energetic and massive molecular cloud with a striking 'whirlpool-esque' morphology, as revealed by ACES observations of the HNCO (4-3) line. The authors explore potential theories behind the unique morphology of the molecular cloud, including the possible roles of stellar feedback, cloud-cloud collisions, and large-scale dynamics. Nonhebel et. al (2024) concludes that the most likely explanation behind the M0.8-0.2 Ring is an explosion of an abnormally luminous supernova, or 'hypernova', embedded deep within a molecular cloud.

Contributed by Mairi Nonhebel

 


Results from October's poll, "Have you considered submitting a joint observatory proposal?"
 

Survey results


 

Did you know?

The Nordic ALMA Node has developed UVMultiFit, a versatile library implemented in CASA for fitting models directly to visibility data. Visibility fitting is a powerful method to analyse interferometric data and extract source information without image deconvolution. You can find an I-TRAIN video tutorial demonstrating how to use it.


If you would like to contribute an ALMA science highlight, please contact the newsletter editor at Hannah.Stacey@eso.org.