SMSS J0313−6708
Mass~0.8 M☉
Distance6,000 ly
TypeK giant
Devesh Nandal is a Swiss National Science Foundation Postdoctoral Fellow at the Center for Astrophysics | Harvard & Smithsonian, studying stellar evolution, the first stars, black hole formation, and their observable signatures in the early Universe.
Mass~0.8 M☉
Distance6,000 ly
TypeK giant
Mass~215 M☉
Distance163,000 ly
TypeWN5h
Mass~100 M☉
Distance7,500 ly
TypeLBV
Mass0.75 M☉
Distance200 ly
TypeG0 IV–V
Mass~15 M☉
Distance~640 ly
TypeM1–2 Ia–ab
Mass2.06 M☉
Distance8.6 ly
TypeA1 V
Mass~0.12 M☉
Distance4.25 ly
TypeM5.5 Ve
Mass~20 M☉
Distance~860 ly
TypeB8 Ia
Mass~16 M☉
Distance~9,500 ly
TypeWO2
His research develops next generation stellar evolution models across extreme stellar masses, with a focus on rotation, angular momentum transport, accretion, mass loss and advanced evolution. These models connect the physics of the first stars to chemical enrichment, black hole formation, and signatures observable with JWST.
Four connected research themes spanning stellar evolution, the first stars, dark matter and the observable signatures of the early Universe.
Testing whether primordial supermassive stars can reproduce the spectra, luminosities and compact gas structures of JWST's enigmatic Little Red Dots.
Read the CfA feature
How supermassive stars form, grow and evolve through accretion, rotation, collisions and mass loss before producing massive black hole seeds.
Explore the models
Rotating metal-free stars across 5 to 200 solar masses, followed through advanced burning to connect internal transport, final fates and nucleosynthetic yields.
View the Pop III grid
Using nitrogen, carbon, oxygen and neon abundances in high-redshift galaxies to identify the stellar populations that enriched the early Universe.
See the GS 3073 resultConnecting the physics of the first stars to the chemical, radiative and black hole signatures now emerging from the early Universe.
SUMER
Explore stellar evolution through graphs, model comparisons and visual research notes, from the lives of massive stars to the early universe.
A visual sketch of how a model star's luminosity can evolve over time.
Compare relative lifetimes across a set of example stellar models.
Conversations, lectures, interviews and explorations of the cosmos.
The James Webb Space Telescope mission team explains how Webb looks back at the earliest galaxies.
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Watch on YouTube ↗Public astronomy explainers from NASA and the Webb mission team.
The James Webb Space Telescope mission team explains how Webb looks back at the earliest galaxies.
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Watch on YouTube ↗NASA introduces the observatory exploring stars, distant galaxies and the early universe.
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Watch on YouTube ↗Explore the telescope revealing the earliest chapters of cosmic history.
NASA's film trailer follows the telescope built to peer billions of years into the past.
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Watch on YouTube ↗Open research reviews on the first stars and black-hole seeds.
Volker Bromm's research review of primordial star formation and Population III stellar systems.
A research review by Lionel Haemmerle and collaborators on cosmic dawn, the first stellar populations and early black-hole seeds.
Swiss National Science Foundation Postdoctoral Fellow · Center for Astrophysics.
Building physical models and connecting predictions to distant observations.
Exploring how the earliest massive stars may have shaped cosmic history.
For research conversations, collaborations, seminars and scientific opportunities.