Home
Astronomy research
Software Infrastructure:
MESA
FLASH
STARLIB
MESA-Web
starkiller-astro
My instruments
White dwarf supernova:
Remnant metallicities
Colliding white dwarfs
Merging white dwarfs
Ignition conditions
Metallicity effects
Central density effects
Detonation density effects
Tracer particle burning
Subsonic burning fronts
Supersonic burning fronts
W7 profiles
Massive star supernova:
Rotating progenitors
3D evolution
26Al & 60Fe
44Ti, 60Co & 56Ni
Yields of radionuclides
Effects of 12C +12C
SN 1987A light curve
Constraints on Ni/Fe ratios
An r-process
Neutron Stars and Black Holes:
Black Hole Mass Gap
Compact object IMF
Stars:
Neutrino HR diagram
Pulsating white dwarfs
Pop III with JWST
Monte Carlo massive stars
Neutrinos from pre-SN
Pre-SN variations
Monte Carlo white dwarfs
SAGB stars
Classical novae
He shell convection
Presolar grains
He burn on neutron stars
BBFH at 40 years
Chemical Evolution:
Iron Pseudocarbynes
Radionuclides in the 2020s
Hypatia catalog
Zone models H to Zn
Mixing ejecta
γ-rays within 100 Mpc
Thermodynamics & Networks
Stellar EOS
12C(α,γ)16O Rate
Proton-rich NSE
Reaction networks
Bayesian reaction rates
Verification Problems:
Validating an astro code
Su-Olson
Cog8
Mader
RMTV
Sedov
Noh
Software instruments
Presentations
Illustrations
cococubed YouTube
Bicycle adventures
Public Outreach
Education materials
2022 ASU Solar Systems Astronomy
2022 ASU Energy in Everyday Life
AAS Journals
AAS YouTube
2022 Earendel, A Highly Magnified Star
2022 TV Columbae, Micronova
2022 White Dwarfs and 12C(α,γ)16O
2022 MESA in Don't Look Up
2022 MESA Marketplace
2022 MESA Summer School
2022 MESA Classroom
2021 Bill Paxton, Tinsley Prize
Contact: F.X.Timmes
my one page vitae,
full vitae,
research statement, and
teaching statement.
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The
W7
zone masses, and density and temperature history of each zone mass are in this
w7_profiles.zip file courtesy Friedel Thielemann circa 2001.
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