1974
DOI: 10.1086/152775
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Infrared fluxes spectral types and temperatures for very cool stars.

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Cited by 40 publications
(43 citation statements)
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“…The effective temperature accompanying each spectral type are from Ridgeway et al (1980). Using bolometric corrections BC K obtained from Dyck et al (1974), wefind excellent agreement between Johnson et al (1980) and Ridgeway et al (1980) when the data are compared using Equations ib and ic.…”
Section: Q Values: Theory and Observationsupporting
confidence: 71%
“…The effective temperature accompanying each spectral type are from Ridgeway et al (1980). Using bolometric corrections BC K obtained from Dyck et al (1974), wefind excellent agreement between Johnson et al (1980) and Ridgeway et al (1980) when the data are compared using Equations ib and ic.…”
Section: Q Values: Theory and Observationsupporting
confidence: 71%
“…The PACS (blue dots) and SPIRE (cyan dots) spectra are also plotted when available. The published photometric data (open circles) are taken from Dyck et al (1974) and Epchtein et al (1980) for WX Psc, Persi et al (1990) for OH 127.8+0.0, Garcia-Lario et al (1997) and Lepine et al (1995) for AFGL 5379, Werner et al (1980) for OH 26.5+0.6, and Justtanont et al (2006) for both OH 26.5+0.6 and OH 30.1-0.7.…”
Section: Wx Psc (Irc+10011)mentioning
confidence: 99%
“…As it has not been detected in any radio lines, we adopt the radial velocity determined optically (General Catalogue of Stellar Radial Velocities, GCRV). Adopting the effective temperature scale for Mira variables of Dyck et al (1974), T eff should be around 3400 K.…”
Section: Oxygen-rich Agb Sourcesmentioning
confidence: 99%