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Morphology, kinematics and star form...

Erroz-Ferrer, Santiago.

Morphology, kinematics and star formation across the Hubble sequence of galaxies

Record Type:	Electronic resources : Monograph/item
Title/Author:	Morphology, kinematics and star formation across the Hubble sequence of galaxiesby Santiago Erroz-Ferrer.
Author:	Erroz-Ferrer, Santiago.
Published:	Cham :Springer International Publishing :2016.
Description:	xiii, 201 p. :ill. (some col.), digital ;24 cm.
Contained By:	Springer eBooks
Subject:	Physics.
Online resource:	http://dx.doi.org/10.1007/978-3-319-26398-4
ISBN:	9783319263984$q(electronic bk.)

Morphology, kinematics and star formation across the Hubble sequence of galaxies
Erroz-Ferrer, Santiago.

Morphology, kinematics and star formation across the Hubble sequence of galaxies[electronic resource] /by Santiago Erroz-Ferrer. - Cham :Springer International Publishing :2016. - xiii, 201 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Massive star formation in galaxies with excess UV emission -- H_ kinematics of S4G spiral galaxies: The data -- Streaming motions in the spiral galaxy NGC 864 -- Non-circular motions and star formation in S4G galaxies -- Inner rotation curves -- Conclusions and future work.

This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies.

ISBN: 9783319263984$q(electronic bk.)

Standard No.: 10.1007/978-3-319-26398-4doiSubjects--Topical Terms:

179414
Physics.

LC Class. No.: QB4

Dewey Class. No.: 520

Morphology, kinematics and star formation across the Hubble sequence of galaxies
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300 $a xiii, 201 p. : $b ill. (some col.), digital ; $c 24 cm.
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505 0 $a Introduction -- Massive star formation in galaxies with excess UV emission -- H_ kinematics of S4G spiral galaxies: The data -- Streaming motions in the spiral galaxy NGC 864 -- Non-circular motions and star formation in S4G galaxies -- Inner rotation curves -- Conclusions and future work.
520 $a This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies.
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