Rotating massive stars: From first stars to gamma ray bursts

By Andre Maeder, G. Meynet. 2012

149 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Instrumentation

View Paper: https://www.semanticscholar.org/paper/e7f509d183778eec03395f5c5126e2fd495e8838

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. N. Langer
2. C. Conroy
3. R. Hirschi
4. G. Meynet
5. M. Limongi
6. A. Chieffi
7. Stan Woosley
8. S. Ekström

In Instrumentation

1. C. Conroy
2. N. Langer
3. Benjamin D. Johnson
4. A. Chieffi
5. M. Limongi
6. R. Hirschi
7. Aaron Dotter
8. S. Ekström

Citations in the corpus

• Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death (2013, background): “Mass loss and angular momentum evolution play a key role in determining the properties of massive stars across their evolution and the properties of the SN progenitor and the ensuing explosion (for recent reviews see Maeder & Meynet 2012; Langer 2012).”
• Binarity in carbon-enhanced metal-poor stars (2014, background): “…and/or wind ejecta of Pop III stars where rotation of these stars plays a major role (e.g., Fryer, Woosley & Heger 2001; Meynet, Ekström & Maeder 2006; Chiappini et al. 2006; Karlsson 2006; Hirschi 2007; Chiappini et al. 2008; Meynet et al. 2010; Maeder & Meynet 2012; Cescutti et al. 2013).”
• MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS (2016, background): “These observed numbers come from Table 2 of Maeder & Meynet (2012), which is 25 While gravitational settling works against these processes, it is a slow process with a negligible effect in the presence of rapid rotation.”
• Chemical evolution with rotating massive star yields - I. The solar neighbourhood and the s-process elements (2018, background): “Also, as the surface rotational velocity approaches the critical one, the mass loss rate is largely enhanced (the ”mechanical” wind discussed, e.g., by Maeder & Meynet 2012 and references therein) but this phenomenon plays an important role only if the surface velocity gets very close to the…”
• Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants (2012, background): “The effects of rotation and in particular the transport of chemicals and angular momentum by meridional circulation and shear instability have been included in stellar evolution codes (see the review by Maeder & Meynet 2012).”
• Evolution and fate of very massive stars (2013, methodology): “(vii) The treatment of rotation in the GENEVA code has been described in Maeder & Meynet (2012).”
• Classical Be stars (2013, background): “It has been suggested that their rapid rotation has some connection to long gamma ray bursts (see, e.g., Woosley and Bloom 2006; Martayan et al. 2010b; Maeder and Meynet 2012).”
• Modeling the Panchromatic Spectral Energy Distributions of Galaxies (2013, background): “The importance of stellar rotation has been investigated by the Geneva group, amongst others, over the past two decades (see Maeder & Meynet 2000, 2012, for a review).”
• Physical Processes in the Interstellar Medium (2014, background): “…also note that stellar rotation can dramatically change the derived stellar mass loss rates and the energy and momentum inserted by line-driven winds (for recent reviews, see Meynet 2009 or Maeder & Meynet 2012, or for a grid of evolutionary tracks, see Ekström et al. 2012 and Georgy et al. 2012).”
• A new route towards merging massive black holes (2016, background): “…physics of the evolution of massive stars, although there are still significant uncertainties, for instance, in the treatment of stellar winds (Langer 2012), rotational mixing (Maeder & Meynet 2012), and the BH formation itself (Heger et al. 2003; Ugliano et al. 2012; Pejcha & Thompson 2015).”
• Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range −3 ≤ [Fe/H] ≤ 0 (2018, background): “…et al. 2000; Meynet & Maeder 2003; Heger et al. 2005; Meynet & Maeder 2005; Brott et al. 2011; Limongi & Chieffi 2012; Chieffi & Limongi 2013; Maeder & Meynet 2012; Ekström et al. 2012), a homogeneous and extended set (in mass, metallicity, initial rotation velocity, and number of nuclear…”
• THE EFFECTS OF STELLAR ROTATION. II. A COMPREHENSIVE SET OF STARBURST99 MODELS (2014, background): “Maeder & Meynet (2000, 2012) reviewed the fundamental physical processes associated with massive star rotation.”