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Asteroseismology from Equivalent Widths: A Test of the Sun

Published online by Cambridge University Press:  08 February 2017

C.U. Keller ,
J.W. Harvey ,
S.C. Barden ,
M.S. Giampapa ,
F. Hill  and
C.A. Pilachowski
C.U. Keller
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA
J.W. Harvey
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA
S.C. Barden
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA
M.S. Giampapa
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA
F. Hill
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA
C.A. Pilachowski
Affiliation:
National Optical Astronomy Observatories, P. O. Box 26732, Tucson, AZ 86726-6732, USA

Extract

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Kjeldsen et al. (1995) reported a probable detection of solar-like, low-amplitude p-mode oscillations in η Bootes using equivalent width measurements from low-resolution spectra of hydrogen Balmer lines. However, this detection has not been confirmed so far. Indeed, there is no confirmed detection of p-mode oscillations in a solar-like star using the equivalent width technique or any other approach (Bedding 1998).

Type
VI. Asteroseismology II
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 375 - 378
Copyright
Copyright © Kluwer 1998 

References

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