大葉大學圖書館 |

Radial-velocity searches for planets around active stars[electronic resource] /

紀錄類型:	書目-電子資源 : Monograph/item
杜威分類號:	523.8
書名/作者:	Radial-velocity searches for planets around active stars/ by Raphaelle D. Haywood.
作者:	Haywood, Raphaelle D.
出版者:	Cham : : Springer International Publishing :, 2016.
面頁冊數:	xv, 140 p. : : ill., digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Stars with planets.
標題:	Extrasolar planets - Detection.
標題:	Orbital mechanics.
標題:	Physics.
標題:	Astronomy, Observations and Techniques.
標題:	Astrophysics and Astroparticles.
標題:	Extraterrestrial Physics, Space Sciences.
標題:	Astrobiology.
ISBN:	9783319412733
ISBN:	9783319412726
內容註:	Introduction: the Hunt for Extra-solar Planets -- A Toolkit to Detect Planets Around Active Stars -- Application to Observations of Planet-hosting Stars -- An Exploration into the Radial-velocity Variability of the Sun -- Conclusion.
摘要、提要註:	This thesis develops new and powerful methods for identifying planetary signals in the presence of "noise" generated by stellar activity, and explores the physical origin of stellar intrinsic variability, using unique observations of the Sun seen as a star. In particular, it establishes that the intrinsic stellar radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields. With the advent of powerful telescopes and instruments we are now on the verge of discovering real Earth twins in orbit around other stars. The intrinsic variability of the host stars themselves, however, currently remains the main obstacle to determining the masses of such small planets. The methods developed here combine Gaussian-process regression for modeling the correlated signals arising from evolving active regions on a rotating star, and Bayesian model selection methods for distinguishing genuine planetary signals from false positives produced by stellar magnetic activity. The findings of this thesis represent a significant step towards determining the masses of potentially habitable planets orbiting Sun-like stars.
電子資源:	http://dx.doi.org/10.1007/978-3-319-41273-3

Radial-velocity searches for planets around active stars[electronic resource] /
Haywood, Raphaelle D.

Radial-velocity searches for planets around active stars[electronic resource] /by Raphaelle D. Haywood. - Cham :Springer International Publishing :2016. - xv, 140 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction: the Hunt for Extra-solar Planets -- A Toolkit to Detect Planets Around Active Stars -- Application to Observations of Planet-hosting Stars -- An Exploration into the Radial-velocity Variability of the Sun -- Conclusion.

This thesis develops new and powerful methods for identifying planetary signals in the presence of "noise" generated by stellar activity, and explores the physical origin of stellar intrinsic variability, using unique observations of the Sun seen as a star. In particular, it establishes that the intrinsic stellar radial-velocity variations mainly arise from suppression of photospheric convection by magnetic fields. With the advent of powerful telescopes and instruments we are now on the verge of discovering real Earth twins in orbit around other stars. The intrinsic variability of the host stars themselves, however, currently remains the main obstacle to determining the masses of such small planets. The methods developed here combine Gaussian-process regression for modeling the correlated signals arising from evolving active regions on a rotating star, and Bayesian model selection methods for distinguishing genuine planetary signals from false positives produced by stellar magnetic activity. The findings of this thesis represent a significant step towards determining the masses of potentially habitable planets orbiting Sun-like stars.

ISBN: 9783319412733

Standard No.: 10.1007/978-3-319-41273-3doiSubjects--Topical Terms:

666954
Stars with planets.

LC Class. No.: QB820

Dewey Class. No.: 523.8

Radial-velocity searches for planets around active stars[electronic resource] /
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