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Astronomy and Astrophysics, ISSN 0004-6361, 01/2016, Volume 585, p. A65
Context. Massive stars likely form by accretion and the evolutionary track of an accreting forming star corresponds to what is called the birthline in the... 
Stars: evolution | Accretion | Stars: formation | accretion disks | stars: evolution | accretion, accretion disks | OBJECTS | MAIN-SEQUENCE | DISTRIBUTIONS | stars: formation | PRIMORDIAL STELLAR EVOLUTION | RATES | PHASE | COLLAPSE | CLOUDS | ASTRONOMY & ASTROPHYSICS | PROTOSTARS | BIRTHLINE | Inflation | Tracking | Stars | Stellar evolution | Entropy | Derivatives | Massive stars | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 403, Issue 1, pp. 45 - 60
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2018, Volume 479, Issue 4, pp. 4544 - 4559
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 12/2019, Volume 490, Issue 2, pp. 2706 - 2716
The first galaxies forming a few hundred million years after the big bang are the key drivers of cosmic evolution and ideal laboratories to study theories of... 
POPULATION | 1ST STARS | methods: numerical | early Universe | LOW-METALLICITY | FRAGMENTATION | RADIATION | cosmology: theory | STREAMING VELOCITIES | BLACK-HOLE FORMATION | IMPACT | ASTRONOMY & ASTROPHYSICS | DARK-MATTER | PRIMORDIAL GAS
Journal Article