Bibcode
DOI
Bilir, S.; Cabrera-Lavers, A.; Karaali, S.; Ak, S.; Yaz, E.; López-Corredoira, M.
Bibliographical reference
Publications of the Astronomical Society of Australia, Volume 25, Issue 2, pp. 69-84.
Advertised on:
0
2008
Citations
44
Refereed citations
43
Description
We estimated the Galactic model parameters for a set of 36 high-latitude
fields included in the currently available Data Release 5 (DR 5) of the
Sloan Digital Sky Survey (SDSS), to explore their possible variation
with the Galactic longitude. The thick disc scaleheight moves from
˜550 pc at 120°
Related projects
Morphology and dynamics of the Milky Way
This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way pretends to provide a data base for the stellar distribution in the most remote and heavily obscured regions of our Galaxy, through the development of semiempirical models based on the
Traces of Galaxy Formation: Stellar populations, Dynamics and Morphology
We are a large, diverse, and very active research group aiming to provide a comprehensive picture for the formation of galaxies in the Universe. Rooted in detailed stellar population analysis, we are constantly exploring and developing new tools and ideas to understand how galaxies came to be what we now observe.
Ignacio
Martín Navarro