The Nature and Evolution of Disks Around Hot Stars

By R. Ignace, K. Gayley. 2005

176 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/f75ba2e970a9807ae70cf685d7182d3e6ca195de

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Citations in the corpus

• Star and Protoplanetary Disk Properties in Orion's Suburbs (2009, methodology): “Effective temperatures, model atmospheres, and extinction We transformed the spectral types to effective temperatures using the relation given by Kenyon & Hartmann (1995) for stars with spectral types earlier than M0, and those by Luhman et al. (2003) for stars of type later than M0.”
• Dynamical mass of the O-type supergiant in ζ Orionis A (2013, background): “Other examples for such rapidly rotatingβCephei stars include πAqr (Peters & Gies 2005) andδSco (Smith 1986).”
• Effects of rotation on the evolution of primordial stars (2008, background): “In that case, the outer layers are no longer bound and some mass is lost, probably through a decretion disc (Owocki 2005) that may be quickly erased by the radiation.”