The Formation and Evolution of M33 as Revealed by Its Star Clusters

This thesis represents the first wide-field photometric and spectroscopic survey of star clusters in the nearby late-spiral galaxy M33. This system is the nearest example of a dwarf spiral galaxy, which may have a unique role in the process of galaxy formation and evolution. The cold dark matter par...

Πλήρης περιγραφή

Λεπτομέρειες βιβλιογραφικής εγγραφής
Κύριος συγγραφέας: San Roman, Izaskun (Συγγραφέας)
Συγγραφή απο Οργανισμό/Αρχή: SpringerLink (Online service)
Μορφή: Ηλεκτρονική πηγή Ηλ. βιβλίο
Γλώσσα:English
Έκδοση: New York, NY : Springer New York : Imprint: Springer, 2013.
Σειρά:Springer Theses, Recognizing Outstanding Ph.D. Research,
Θέματα:
Διαθέσιμο Online:Full Text via HEAL-Link
LEADER 03091nam a22005295i 4500
001 978-1-4614-7327-5
003 DE-He213
005 20151030051143.0
007 cr nn 008mamaa
008 130509s2013 xxu| s |||| 0|eng d
020 |a 9781461473275  |9 978-1-4614-7327-5 
024 7 |a 10.1007/978-1-4614-7327-5  |2 doi 
040 |d GrThAP 
050 4 |a QB1-991 
050 4 |a QB460-466 
050 4 |a QB980-991 
072 7 |a PGC  |2 bicssc 
072 7 |a SCI004000  |2 bisacsh 
072 7 |a SCI005000  |2 bisacsh 
082 0 4 |a 520  |2 23 
100 1 |a San Roman, Izaskun.  |e author. 
245 1 4 |a The Formation and Evolution of M33 as Revealed by Its Star Clusters  |h [electronic resource] /  |c by Izaskun San Roman. 
264 1 |a New York, NY :  |b Springer New York :  |b Imprint: Springer,  |c 2013. 
300 |a XVI, 129 p.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
347 |a text file  |b PDF  |2 rda 
490 1 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5053 
505 0 |a Foreword from Professor Ata Sarajedini -- Introduction -- Newly Identified Star Clusters in M33: Space-Based Survey -- Photometric Properties of the M33 Star Cluster System: Ground-Based Survey -- Structural Parameters of the M33 Star Cluster System -- Kinematic Properties of Star Clusters in M33 -- Conclusions. 
520 |a This thesis represents the first wide-field photometric and spectroscopic survey of star clusters in the nearby late-spiral galaxy M33. This system is the nearest example of a dwarf spiral galaxy, which may have a unique role in the process of galaxy formation and evolution. The cold dark matter paradigm of galaxy formation envisions large spiral galaxies, such as the Milky Way, being formed from the merger and accretion of many smaller dwarf galaxies. The role that dwarf spiral galaxies play in this process is largely unclear. One of the goals of this thesis is to use the star cluster population of M33 to study its formation and evolution from its early stages to the present. The thesis presents a new comprehensive catalog of M33 star clusters, which includes magnitudes, colors, structural parameters, and several preliminary velocity measurements. Based on an analysis of these data, the thesis concludes that, among other things, the evolution of M33 has likely been influenced by its nearby massive neighbor M31. 
650 0 |a Physics. 
650 0 |a Astronomy. 
650 0 |a Astrophysics. 
650 0 |a Cosmology. 
650 0 |a Spectroscopy. 
650 0 |a Microscopy. 
650 1 4 |a Physics. 
650 2 4 |a Astronomy, Astrophysics and Cosmology. 
650 2 4 |a Spectroscopy and Microscopy. 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer eBooks 
776 0 8 |i Printed edition:  |z 9781461473268 
830 0 |a Springer Theses, Recognizing Outstanding Ph.D. Research,  |x 2190-5053 
856 4 0 |u http://dx.doi.org/10.1007/978-1-4614-7327-5  |z Full Text via HEAL-Link 
912 |a ZDB-2-PHA 
950 |a Physics and Astronomy (Springer-11651)