Improved opacities and pulsation stability in subluminous B and O stars

Monthly Notices of the Royal Astronomical Society

Volumn 378, Issue 1, 2007, Pages 379-383

  Jeffery, C S ^a,b   Saio, H ^a,b  

^a ARMAGH OBSERVATORY   (United Kingdom)

^b TOHOKU UNIVERSITY   (Japan)

Author keywords

Atomic processes; Radiative transfer; Stars: early type; Stars: horizontal branch; Stars: interiors; Stars: oscillations

Indexed keywords

IRON; NICKEL; STABILITY; STARS; TEMPERATURE;

ATOMIC PROCESS; EARLY-TYPE - STARS; EFFECTIVE TEMPERATURE; LOW ORDER; LOW-MASS; RADIAL OSCILLATION; STAR OSCILLATIONS; STARS: HORIZONTAL BRANCH; STARS: INTERIORS; STARS:EARLY TYPE;

OPACITY;

EID: 34249679179     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11794.x     Document Type: Article

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