Michelle Collins
@runningastronomer.bsky.social
5.8K followers 910 following 880 posts
✨Astronomer searching for and studying the faintest galaxies in the Universe ✨co-host of the @starxiv.bsky.social podcast ✨ Enthusiastic-but-mediocre runner 🏃🏻‍♀️ vegan 🌱 She/her
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runningastronomer.bsky.social
Tomorrow it is world space week on Guildford high Street! Join us from 10-4 for space, science, planets, galaxies, stars and satellites! I can't wait ☄️🌕👽🌟🛰️🛸👩🏻‍🚀🧪🔭
an astronaut in a space suit is flying through space
Alt: an astronaut in a space suit is flying through space
media.tenor.com
runningastronomer.bsky.social
Cordoba is lovely, by the way 🤩
Me and Duncan Forbes, posing amidst the red and white striped arches of the Mesquita The main altar of the cathedral found within Cordoba's mosque. A wider view of the arches and pillars of the Mesquita
runningastronomer.bsky.social
Have you heard last week's episode of the Starxiv yet? It's a great one! Episode 22 will be released next Monday but I won't be in it as this week I'm in Cordoba for a conference on galaxy outskirts ☄️🔭
starxiv.bsky.social
Episode 21 is live! Tune in to here the latest results on Mercury's magnetosphere, population III stars, relic galaxies, quasi-periodic eruptions and more, with your hosts, Michelle and Nicole. Available on our website, Spotify, Apple, or wherever you get podcasts 🔭 ☄️
starxiv.com
Reposted by Michelle Collins
jradavenport.com
If anyone from the UN wants to talk, here’s a nice summary. The astronomy community does NOT endorse this proposal, just take it from one of THE EXPERTS on ISOs with Rubin. Meg (and many others) has helped the community plan for +10yrs for these kinds of studies.
megschwamb.bsky.social
I'll for global coordination for ISO follow-up, but it's telling that no one who's actually coordinating follow-up was actually asked to participate in this proposal or thought of to be even suggested as names on committees in this proposal
runningastronomer.bsky.social
I literally sang this to myself repeatedly during the last HST cycle 😂
Reposted by Michelle Collins
lsstuk.bsky.social
An exciting and positive read – we're happy to see the piece give a shoutout to rising talent in #astronomy, including Astha whom we interviewed recently about her LSST:UK work too.
runningastronomer.bsky.social
Great article featuring some of our Surrey astrophysics students! Unfortunately they seem to have been attributed to the wrong supervisor, but wonderful to see them talking passionately about the work they are doing with @payeldas.bsky.social @derkal.bsky.social and Noelia Noël 🔭☄️🧪
davidbflower.bsky.social
Can a satellite unlock the secrets of the universe? 🔭 🧪 www.bbc.co.uk/news/article...
runningastronomer.bsky.social
Great article featuring some of our Surrey astrophysics students! Unfortunately they seem to have been attributed to the wrong supervisor, but wonderful to see them talking passionately about the work they are doing with @payeldas.bsky.social @derkal.bsky.social and Noelia Noël 🔭☄️🧪
Reposted by Michelle Collins
starxiv.bsky.social
Nicole’s final paper discussed this new take on second-gen (G2) stars in globular clusters: maybe they weren’t born polluted… maybe they merged into it. Mergers of MS + HeWD binaries can produce G2-like stars with He and N enrichment — even in the field.
arxiv.org/abs/2509.15337 🔭☄️
Left panel: optical CMD, namely F555W-(F439W-F555W), of the globular cluster NGC 362 based on HST photometry from Piotto et al. (2002); three red filled squires show the expected consecutive locations of an initial MS binary in its evolution toward RGB-like merger remnant, schematically shown in the right panel; the blue points show the stars of the RGB in its total range beginning from the RGB base. Right panel: schematic illustration of the main consecutive stages of the evolution of a hard binary initially composed of two MS stars (1), then converted into a (MSS+HeWD) binary (2), which finally merges forming RGB-like merger product (3) evolving along the cluster RGB.
Reposted by Michelle Collins
royalastrosoc.bsky.social
Today marks the start of '100 Hours of Astronomy'! 🔭🪐💫

Want to take part in the global stargazing event? Join in any time from now until Sunday by completing four simple challenges to find star patterns and a planet in the night sky.

Find out more at: 100hours.online
runningastronomer.bsky.social
This episode I learnt about quasi periodic eruptions, mysterious bursts of x rays emanating from near super massive black holes. What causes then? Tune in to hear one theory about this 🔭☄️🧪
starxiv.bsky.social
In Michelle's second paper, we learned about quasi-periodic eruptions from Ansky and what might generate them. In this case, new monitoring shows that the period and intensity of Ansky's QPEs are increasing, but why? Tune in to find out ☄️ 🔭 !https://arxiv.org/abs/2509.16304
Data showing the flare profiles measured in 2024 and 2025. The luminosity and period have dramatically increased!
runningastronomer.bsky.social
4-most are here! Check out this cool spectroscopic survey and follow their progress. The science will be amazing!!! First light coming VERY soon
4most-eu.bsky.social
Welcome to the official 4-metre Multi-Object Spectroscopic Telescope (4MOST) Bluesky account! Stay tuned for our first-light events coming very soon, and updates on all of the amazing science we will be completing over the years to come!

📷: Y. Beletsky/ESO

#4most #ESO #telescope #astronomy
runningastronomer.bsky.social
How much mixing happens at early times in the universe? And will it be a problem when using chemical tagging to investigate galaxy build up? Nicole talked us through it in our latest episode 🧪☄️🔭
starxiv.bsky.social
Nicole talked about early metal mixing with Aeos, a sim of Pop III enrichment. Gas is only chemically coherent within 100 pc and 7 Myr after a SN. Beyond that, stars form with distinct abundance patterns. This Mahalanobis distance plot shows this divergence.
arxiv.org/abs/2509.13580 🔭☄️
Top: Number of stars per time bin. Bottom: dM along with 16th to 84th percentile spread of dM over TSF assuming instantaneous and homogeneous mixing across spheres of radius R. (The zero-point of TSF is the time at which each star forms.) Prior to ∼7Myr after a star forms, smaller spheres have smaller dM. The dM for each sphere intersects at ∼7Myr, suggesting τchem=7Myr. After 7Myr, the dM of spheres R≤0.1kpc continues to increase dramatically, consistent with rapidly changing local gas, whereas the dM of spheres R≥0.5kpc flattens, consistent with expectations for an IMF-averaged gas abundance.
runningastronomer.bsky.social
I love how much we can learn about galaxies from deep images like these, and incredible coming from amateur telescopes too🤩 🧪☄️🔭
starxiv.bsky.social
Michelle's first paper discusses the Pearl in the Shell, a study of an ultra compact dwarf and a debris cloud around a nearby spiral galaxy. The study combines data from professional and amatCheck it out in our latest episode! arxiv.org/abs/2509.14038 🔭 ☄️
Amateur image of NGC 7531 (left). DESI Legacy Imaging Survey image of NGC 7531 (right). Sky-subtracted image of NGC 7531 as
processed by Gnuastro’s NoiseChisel program was used as a basis for photometry measurements. Features are labelled: (a): main shell; (b): faint
outer shell; c: counter plume.
Reposted by Michelle Collins
starxiv.bsky.social
Nicole talked about early metal mixing with Aeos, a sim of Pop III enrichment. Gas is only chemically coherent within 100 pc and 7 Myr after a SN. Beyond that, stars form with distinct abundance patterns. This Mahalanobis distance plot shows this divergence.
arxiv.org/abs/2509.13580 🔭☄️
Top: Number of stars per time bin. Bottom: dM along with 16th to 84th percentile spread of dM over TSF assuming instantaneous and homogeneous mixing across spheres of radius R. (The zero-point of TSF is the time at which each star forms.) Prior to ∼7Myr after a star forms, smaller spheres have smaller dM. The dM for each sphere intersects at ∼7Myr, suggesting τchem=7Myr. After 7Myr, the dM of spheres R≤0.1kpc continues to increase dramatically, consistent with rapidly changing local gas, whereas the dM of spheres R≥0.5kpc flattens, consistent with expectations for an IMF-averaged gas abundance.
Reposted by Michelle Collins
starxiv.bsky.social
Episode 21 is live! Tune in to here the latest results on Mercury's magnetosphere, population III stars, relic galaxies, quasi-periodic eruptions and more, with your hosts, Michelle and Nicole. Available on our website, Spotify, Apple, or wherever you get podcasts 🔭 ☄️
starxiv.com
Reposted by Michelle Collins
karenlmasters.bsky.social
Deadline is a week from now, and I'm hoping to hire to start ASAP - the grant period is officially 1st Oct 2025-2027 (I promise I posted the advert as soon as I could after hearing we got funded; how do the rest of you do this to hire for Academic year cycle?).
runningastronomer.bsky.social
Oh no! I'm so sorry, that's awful
Reposted by Michelle Collins
elisecutts.bsky.social
Bad science communication can be disastrous. But a typo clearly isn't as bad as fraud. Clearly, a scale is needed to resolve this ambiguity.

Thus, I here propose the Loeb Scale for scientific PR disasters.

It is NOT to be confused with the recently proposed Loeb Scale for interstellar objects. 🔭
The Loeb Scale for science PR disasters
Science miscommunication is dangerous. But how dangerous?
www.reviewertoo.com
Reposted by Michelle Collins
stephenserjeant.bsky.social
I'm glad to read this. About time. Also I don't understand why he was made FRS in the first place. He's not a scientist and he's not an engineer. He's a business leader who pontificates wildly on scientific subjects in which he knows next to nothing and his DOGE has actively damaged US science. 🔭🧪
jamesrball.com
Mini-scoop: After resisting pressure to strip Elon Musk of his fellowship for months, the Royal Society is meeting on 1 October to discuss his removal – following his decision to address Tommy Robinson's far-right rally on Saturday.

www.thenewworld.co.uk/james-ball-r...
Royal Society to debate throwing out Elon Musk
One of the most prestigious scientific bodies in the world is considering expelling Musk after his appearance at Tommy Robinson’s extremist London rally
www.thenewworld.co.uk