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Izaskun San Roman - The Formation and Evolution of M33 as Revealed by Its Star Clusters - 9781461473268 - V9781461473268
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The Formation and Evolution of M33 as Revealed by Its Star Clusters

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Description for The Formation and Evolution of M33 as Revealed by Its Star Clusters hardcover. This is the first wide-field photometric and spectroscopic survey of star clusters in the galaxy M33, the nearest example of a dwarf spiral galaxy. Includes data on magnitudes, colors, structural parameters and several preliminary velocity measurements. Series: Springer Theses. Num Pages: 145 pages, 5 black & white tables, biography. BIC Classification: PGC; PGM; PNFS. Category: (P) Professional & Vocational. Dimension: 235 x 155 x 15. Weight in Grams: 391.
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 ... Read more

Product Details

Format
Hardback
Publication date
2013
Publisher
Springer United States
Number of pages
145
Condition
New
Series
Springer Theses
Number of Pages
129
Place of Publication
New York, NY, United States
ISBN
9781461473268
SKU
V9781461473268
Shipping Time
Usually ships in 15 to 20 working days
Ref
99-15

About Izaskun San Roman
Izaskun San Roman was born in Alsasua, Spain. After high school she moved to Tenerife, Canary Islands, where she received her B.S. in physics and astrophysics from the University of La Laguna. While at ULL, she met her husband. She then moved to Gainesville, Florida, to attend graduate school at the University of Florida, where she worked on stellar population ... Read more

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