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Anna Rosen, Ph.D.Computational Astrophysicist
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Interactive

Explore the cluster

Hands-on pieces built on the same physics as my Jaxstro models, reimplemented to run in your browser — for curiosity, for talks, for the classroom. Drag, zoom, and turn the knobs; the physics is honest, not decorative.

  • The cluster census

    Sample a star cluster from the initial mass function and read it two ways at once — as points in space and on the H–R diagram. Every colour, temperature and luminosity is computed live from the same validated ZAMS physics my software uses.

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  • No star is an island

    Switch gravity on and a static scatter becomes a system: energies get shuffled, the heaviest stars sink, and the cluster segregates itself. Integrated in your browser with a symplectic scheme of the family gravax uses — with the energy drift shown, so you can check it.

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  • Gas expulsion

    Massive-star feedback drives the natal gas outward, unbinding the cloud and leaving the young cluster behind. Scrub the expulsion or let it play.

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  • Birth of a cluster

    A turbulent cloud grows dense, ignites its stars, and blows itself clear with feedback — the life of a star cluster, told scroll by scroll from a real gravoturb model.

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  • Inference in progress

    Watch a posterior over a cluster's mass, age, and size tighten as observations arrive — differentiable inference, using informax's method, on a synthetic cluster.

Anna Rosen

Assistant Professor of Astronomy, San Diego State University

alrosen@sdsu.edu

The universe may be cruel, but at least it's consistent.

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Built with Astro. Source on GitHub. Content licensed for reuse with attribution unless noted.