Rights statement: This is an Accepted Manuscript of an article published by Taylor & Francis in Contemporary Physics 2019, available online: https://www.tandfonline.com/doi/abs/10.1080/00107514.2019.1662096.
Accepted author manuscript, 123 KB, PDF document
Final published version
Research output: Contribution to Journal/Magazine › Book/Film/Article review
Research output: Contribution to Journal/Magazine › Book/Film/Article review
}
TY - JOUR
T1 - Asteroseismic data analysis: foundations and techniques
T2 - by Sarbani Basu and William J. Chaplin, Princeton, Princeton University Press, 2017, 337 pp., £58.00 (hardback), ISBN: 978-0-691-16292-8. Scope: textbook. Level: postgraduate students and professional astrophysicists
AU - McClintock, Peter V. E.
N1 - This is an Accepted Manuscript of an article published by Taylor & Francis in Contemporary Physics 2019, available online: https://www.tandfonline.com/doi/abs/10.1080/00107514.2019.1662096.
PY - 2019/9/9
Y1 - 2019/9/9
N2 - Stars pulsate and their nature of their pulsations can provide a great deal of information about them including, for example, their masses, radii and ages. Oscillations in stellar brightness were first observed long ago, at the end of the sixteenth century. Since then, it has been established the phenomenon is seemingly a ubiquitous feature of stars and its study has been named asteroseismology.
AB - Stars pulsate and their nature of their pulsations can provide a great deal of information about them including, for example, their masses, radii and ages. Oscillations in stellar brightness were first observed long ago, at the end of the sixteenth century. Since then, it has been established the phenomenon is seemingly a ubiquitous feature of stars and its study has been named asteroseismology.
U2 - 10.1080/00107514.2019.1662096
DO - 10.1080/00107514.2019.1662096
M3 - Book/Film/Article review
VL - 60
SP - 274
JO - Contemporary Physics
JF - Contemporary Physics
SN - 0010-7514
IS - 3
ER -