LEADER 03507nam 22006375 450 001 9910254608103321 005 20200705033839.0 010 $a3-319-26398-6 024 7 $a10.1007/978-3-319-26398-4 035 $a(CKB)3710000000515872 035 $a(EBL)4101853 035 $a(SSID)ssj0001585340 035 $a(PQKBManifestationID)16265266 035 $a(PQKBTitleCode)TC0001585340 035 $a(PQKBWorkID)14866461 035 $a(PQKB)10649205 035 $a(DE-He213)978-3-319-26398-4 035 $a(MiAaPQ)EBC4101853 035 $a(PPN)190537256 035 $a(EXLCZ)993710000000515872 100 $a20151121d2016 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aMorphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies /$fby Santiago Erroz-Ferrer 205 $a1st ed. 2016. 210 1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2016. 215 $a1 online resource (207 p.) 225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 300 $a"Doctoral thesis accepted by the University of La Laguna, Spain." 311 $a3-319-26397-8 320 $aIncludes bibliographical references at the end of each chapters and index. 327 $aIntroduction -- 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. 330 $aThis thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies. 410 0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053 606 $aObservations, Astronomical 606 $aAstronomy?Observations 606 $aAstrophysics 606 $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014 606 $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022 615 0$aObservations, Astronomical. 615 0$aAstronomy?Observations. 615 0$aAstrophysics. 615 14$aAstronomy, Observations and Techniques. 615 24$aAstrophysics and Astroparticles. 676 $a530 700 $aErroz-Ferrer$b Santiago$4aut$4http://id.loc.gov/vocabulary/relators/aut$0805588 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254608103321 996 $aMorphology, Kinematics and Star Formation Across the Hubble Sequence of Galaxies$91808144 997 $aUNINA