Mass loss from stars and the evolution of stellar clusters : proceedings of a workshop held at Lunteren, The Netherlands 29 May - 1 June 2006

By A. D. Koter, L. Smith, L. Waters. 2008

142 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/f76b0e1fbc7d08398c97aa8ed3adf614c13df56f

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

1. N. Smith
2. K. Hinkle
3. N. Ryde
4. S. Larsen
5. S. Smartt
6. Ryan Chornock
7. N. Bastian
8. Weidong Li

Citations in the corpus

• RED SUPERGIANTS AS POTENTIAL TYPE IIn SUPERNOVA PROGENITORS: SPATIALLY RESOLVED 4.6 μm CO EMISSION AROUND VY CMa AND BETELGEUSE (2008, background): “As emphasized elsewhere (Smith 2008; Smith et al. 2007), continually mounting observational evidence suggests that LBVs or LBV-like stars may explode (Smith & Owocki 2006; Smith et al. 2007, 2008; Gal-Yam et al. 2007; Vink et al. 2008; Kotak & Vink 2006).”
• The mass function of young star clusters in spiral galaxies (2008, methodology): “The MF derived here differs from that obtained by Dowell et al. (2008) who find power-law slopes of α ∼ −1.8 for 105 < M/M < 107 for clusters in a sample of nearby spiral and irregular galaxies.”