大葉大學圖書館 |

Investigating the A-type stars using Kepler data[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	523.84425
書名/作者:	Investigating the A-type stars using Kepler data/ by Simon J. Murphy.
作者:	Murphy, Simon J.
出版者:	Cham : : Springer International Publishing :, 2015.
面頁冊數:	xvii, 204 p. : : ill. (some col.), digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Astroseismology.
標題:	Stellar oscillations.
標題:	Physics.
標題:	Astrophysics and Astroparticles.
標題:	Astronomy, Observations and Techniques.
ISBN:	9783319094175 (electronic bk.)
ISBN:	9783319094168 (paper)
摘要、提要註:	Simon Murphy's thesis has significant impact on the wide use of the revolutionary Kepler Mission data, leading to a new understanding in stellar astrophysics. It first provides a deep characterisation and comparison of the Kepler long cadence and short cadence data, with particular insight into the Kepler reduction pipeline. It then brings together modern reviews of rotation and peculiarities in A-type stars, and their relationship with the pulsating delta Scuti stars. This is the first combined review of these subjects since the classic monograph by Sydney Wolff, "The A stars," was published three decades ago. The thesis presents a novel technique, Super-Nyquist Asteroseismology, that has opened up the asteroseismic study of thousands of Kepler stars. It shows case studies of delta Scuti stars examining amplitude growth, super-Nyquist pulsation, and pulsation in a high-amplitude, population II SX Phoenicis star in a 343-d binary. This work informs our understanding of the relation of rotation to peculiarity, hence has applications to atomic diffusion theory. This is a brilliant thesis written in an elegant and engaging style.
電子資源:	http://dx.doi.org/10.1007/978-3-319-09417-5

Investigating the A-type stars using Kepler data[electronic resource] /
Murphy, Simon J.

Investigating the A-type stars using Kepler data[electronic resource] /by Simon J. Murphy. - Cham :Springer International Publishing :2015. - xvii, 204 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Simon Murphy's thesis has significant impact on the wide use of the revolutionary Kepler Mission data, leading to a new understanding in stellar astrophysics. It first provides a deep characterisation and comparison of the Kepler long cadence and short cadence data, with particular insight into the Kepler reduction pipeline. It then brings together modern reviews of rotation and peculiarities in A-type stars, and their relationship with the pulsating delta Scuti stars. This is the first combined review of these subjects since the classic monograph by Sydney Wolff, "The A stars," was published three decades ago. The thesis presents a novel technique, Super-Nyquist Asteroseismology, that has opened up the asteroseismic study of thousands of Kepler stars. It shows case studies of delta Scuti stars examining amplitude growth, super-Nyquist pulsation, and pulsation in a high-amplitude, population II SX Phoenicis star in a 343-d binary. This work informs our understanding of the relation of rotation to peculiarity, hence has applications to atomic diffusion theory. This is a brilliant thesis written in an elegant and engaging style.

ISBN: 9783319094175 (electronic bk.)

Standard No.: 10.1007/978-3-319-09417-5doiSubjects--Topical Terms:

602956
Astroseismology.

LC Class. No.: QB539.O83

Dewey Class. No.: 523.84425

Investigating the A-type stars using Kepler data[electronic resource] /
LDR:02114nam a2200313 a 4500 001 424783
003 DE-He213
005 20150608112208.0
006 m d
007 cr nn 008maaau
008 151119s2015 gw s 0 eng d
020 $a 9783319094175 (electronic bk.)
020 $a 9783319094168 (paper)
024 7 $a 10.1007/978-3-319-09417-5 $2 doi
035 $a 978-3-319-09417-5
040 $a GP $c GP
041 0 $a eng
050 4 $a QB539.O83
072 7 $a PHVB $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.84425 $2 23
090 $a QB539.O83 $b M978 2015
100 1 $a Murphy, Simon J. $3 602955
245 1 0 $a Investigating the A-type stars using Kepler data $h [electronic resource] / $c by Simon J. Murphy.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2015.
300 $a xvii, 204 p. : $b ill. (some col.), digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
520 $a Simon Murphy's thesis has significant impact on the wide use of the revolutionary Kepler Mission data, leading to a new understanding in stellar astrophysics. It first provides a deep characterisation and comparison of the Kepler long cadence and short cadence data, with particular insight into the Kepler reduction pipeline. It then brings together modern reviews of rotation and peculiarities in A-type stars, and their relationship with the pulsating delta Scuti stars. This is the first combined review of these subjects since the classic monograph by Sydney Wolff, "The A stars," was published three decades ago. The thesis presents a novel technique, Super-Nyquist Asteroseismology, that has opened up the asteroseismic study of thousands of Kepler stars. It shows case studies of delta Scuti stars examining amplitude growth, super-Nyquist pulsation, and pulsation in a high-amplitude, population II SX Phoenicis star in a 343-d binary. This work informs our understanding of the relation of rotation to peculiarity, hence has applications to atomic diffusion theory. This is a brilliant thesis written in an elegant and engaging style.
650 0 $a Astroseismology. $3 602956
650 0 $a Stellar oscillations. $3 602957
650 1 4 $a Physics. $3 171863
650 2 4 $a Astrophysics and Astroparticles. $3 465672
650 2 4 $a Astronomy, Observations and Techniques. $3 464241
710 2 $a SpringerLink (Online service) $3 463450
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 463746
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-09417-5
950 $a Physics and Astronomy (Springer-11651)