E.A. Milne Centre
@EAMilneCentre
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The official Twitter feed for the E.A. Milne Centre for Astrophysics at @UniOfHull 🪐💫
Hull, England
Joined January 2013
Congratulations to friend of the Milne centre @HMO_Stevo !!!🎉🎉.
I am very proud to share that my 2nd first-author paper is now available on arXiv! The paper has also been submitted to MNRAS following the first round of referees report. Quick thread 🧵.
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Congratulations to our Milne staff members, Daniel Farrow and Aoife Curran, and friends!!🎉🎉🎉.
Congratulations DAIM staff Daniel Farrow, Lara Blythe, Aoife Curran & Julius Mboli, for being awarded £4713 from the Ferens Education Trust for “DASSH: Dynamic City: Seismic and Sonic activity in Hull”, a project to teach young learners about seismology, #AI & machine learning.
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🪐Milne Masters Opportunities!📡. Perform numerical hydrodynamical simulations of the combined AGN and merger activity and test how features observed in Hydra A can occur quantitatively with @DrERoediger at the @UniofHull 💫✨.
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🪐Milne Masters Opportunities!📡. Study how the evolution of sloshing cold fronts depends on pre-existing turbulence in the ICM and then compare hydrodynamical simulations to well-observed sloshing clusters with @DrERoediger at the @UniofHull 💫✨.
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🪐Milne Masters Opportunities!📡. Investigate how gas stripping of cluster galaxies depends on ICM turbulence properties using hydrodynamical simulations and comparisons to well-observed examples with @DrERoediger at the @UniofHull!!.
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🪐Milne Masters Opportunities!📡. Stack clusters and groups with @jabberjabber0 to "shed light" on "X-ray dark clusters and groups" by doing an MSc by research at the @UniofHull!!.
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🪐Milne Masters Opportunities!📡. Investigate galaxies in the two sub-classes of Shakhbazyan groups to determine the environmental effect on their evolution with @jabberjabber0 as part of an MSc by research at the @UniOfHull!! .
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🪐Milne Masters Opportunities!📡. Stack clusters and groups with @jabberjabber0 to "shed light" on "X-ray dark clusters and groups" whilst doing an MSc by research at the @UniofHull!!.
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🪐Milne Masters Opportunities!📡. Probe the origin of far-infrared line deficits in galaxies undergoing extreme star formation using state-of-the-art hydrodynamic simulations of isolated disc galaxies with Alex Richings at the @UniofHull!! .
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📡Milne Masters Opportunities!👽. Want to find alien life in the Universe? Join us at the @UniOfHull to start an MSc with @dbenoit1 and reproduce molecular signatures using the Prometheus software. Maybe you'll find some new green friends!.
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You've only got 1 day left to buy tickets for @Jimjam91's talk on "the Lives and Deaths of Stars"!!✨💫. Catch him tomorrow at 5pm in #BeverleyGuildhall!.
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A massive congratulations to the one and only @kate_womack_ who passed her viva yesterday in only 1.5hrs!!🥳😱🥳 . That's gotta be some kind of record!🎉🎉
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RT @RoyalAstroSoc: Good news! 😀. We've extended the deadline to submit nominations for the Caroline Herschel Medal 2025 🏅🏅🏅 . You now have….
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RT @RAS_Journals: Published in #MNRAS: "Atmospheric escape in hot Jupiters under sub-Alfvénic interactions", Presa et al. This is Fig. 1: f….
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RT @UoHHubble: January 2025 Exam Timetable is now live. If you have exams, use the Student Exam Timetable Finder on Sharepoint: https://t.c….
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RT @daimhulluni: Our Director; Prof @jabberjabber0 & Prof Morrell pose the question; 'Can ChatGPT pass a physics degree? Making a case for….
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There's still tickets left to see our very own @Jimjam91 talk about "The Lives and Deaths of Stars" on the 11th of December at #BeverleyGuildhall!!💫✨.
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It's not too late to buy tickets for our Director of the Milne Centre, @DrERoediger's talk "Galaxy Clusters: Shaken and Stirred" at Beverley Guildhall on the 27th of November!! #beverley #hull #Astrophysics . Get your tickets here:.
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We've got new MSc by Research projects available at the @UniOfHull!! . Read about them out at the link below! #MSc #Astrophysics .
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Congratulations to our PhD student, Sophie Eden!! 🎉🎉🎉.
Our ASKAP work led by @EAMilneCentre PhD student, Sophie Eden, just accepted: Galaxies with an impact parameter of <5" are likely to be physically associated with radio sources and are 5x more likely to be an AGN than objects without a radio match.
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