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Science, ISSN 0036-8075, 12/2006, Volume 314, Issue 5805, pp. 1580 - 1583
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 04/2009, Volume 695, Issue 1, pp. L62 - L66
Abundances of C, N, and O are determined in four bright red giants that span the known abundance range for light (Na and Al) and s-process (Zr and La) elements... 
Stars: abundances | Globular clusters: individual (NGC 1851) | Galaxy: abundances
Journal Article
Science, ISSN 0036-8075, 08/2014, Volume 345, Issue 6197, pp. 650 - 653
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 04/2008, Volume 677, Issue 1, pp. 581 - 592
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 4, p. 3866
  The treatment of convective boundaries during core helium burning is a fundamental problem in stellar evolution calculations. In the first paper of this... 
Astrophysics | Luminosity | Stochastic models | Helium | Star & galaxy formation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 456, Issue 4, pp. 3866 - 3866
The treatment of convective boundaries during core helium burning is a fundamental problem in stellar evolution calculations. In the first paper of this... 
Stars | Luminosity | Clumps | Mathematical models | Combustion | Boundaries | Globular clusters | Helium
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 450, Issue 3, p. 2423
  We conduct a series of comparisons between spectroscopic and photometric observations of globular clusters and stellar models to examine their predictive... 
Spectrum analysis | Stars & galaxies | Luminosity | Space telescopes | Comparative analysis | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 450, Issue 3, pp. 2423 - 2423
We conduct a series of comparisons between spectroscopic and photometric observations of globular clusters and stellar models to examine their predictive... 
Spectroscopy | Metallicity | Clusters | Luminosity | Lithium | Mathematical models | Globular clusters | Photometry
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 1, p. 123
  The detection of mixed oscillation modes offers a unique insight into the internal structure of core helium burning (CHeB) stars. The stellar structure... 
Astrophysics | Hydrogen | Pulsars | Cosmology | Helium | Star & galaxy formation | Asymptotic methods
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 1, pp. 123 - 123
The detection of mixed oscillation modes offers a unique insight into the internal structure of core helium burning (CHeB) stars. The stellar structure during... 
Oscillation modes | Asymptotic properties | Stars | Mathematical models | Combustion | Helium | Stellar structure | Pulsation
Journal Article
Astrophysical Journal (Online), ISSN 1538-4357, 04/2009, Volume 695, Issue 1
Abundances of C, N, and O are determined in four bright red giants that span the known abundance range for light (Na and Al) and s-process (Zr and La) elements... 
ALUMINIUM | SODIUM | CARBON | ELEMENT ABUNDANCE | S PROCESS | ASYMPTOTIC SOLUTIONS | MIXTURES | OXYGEN | ZIRCONIUM | GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE | NITROGEN | GALAXIES | GIANT STARS | LANTHANUM
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2009, Volume 695, Issue 1, pp. L62 - L66
Abundances of C, N, and O are determined in four bright red giants that span the known abundance range for light (Na and Al) and s-process (Zr and La) elements... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 3, p. 2804
  There is now strong evidence that some stars have been born with He mass fractions as high as Y ... 0.40 (e.g. in ... Centauri). However, the advanced... 
Helium | Star & galaxy formation | Astronomy
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2015, Volume 452, Issue 3, pp. 2804 - 2804
There is now strong evidence that some stars have been born with He mass fractions as high as Y ... 0.40 (e.g. in ... Centauri). However, the advanced... 
Metallicity | Asymptotic properties | Neutron sources | Stars | Evolution | Stellar evolution | Capture (nuclear) | Lead (metal)
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 446, Issue 3, p. 2599
  We explore the final fates of massive intermediate-mass stars by computing detailed stellar models from the zero-age main sequence until near the end of the... 
Neutron stars | Giant stars | Supernovae | Carbon | Astronomy | White dwarfs
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 446, Issue 3, pp. 2599 - 2599
We explore the final fates of massive intermediate-mass stars by computing detailed stellar models from the zero-age main sequence until near the end of the... 
White dwarf stars | Metallicity | Computation | Supernovas | Combustion | Asymptotic giant branch stars | Carbon | Channels
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2015, Volume 452, Issue 1, pp. 123 - 145
Journal Article
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