Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Westfall, K. B."'
Autor:
Nevin, R., Blecha, L., Comerford, J., Greene, J. E., Law, D. R., Stark, D. V., Westfall, K. B., Vázquez-Mata, J. A., Smethurst, R., Argudo-Fernández, M., Brownstein, J. R., Drory, N.
To determine the importance of merging galaxies to galaxy evolution, it is necessary to design classification tools that can identify different types and stages of merging galaxies. Previously, using GADGET-3/SUNRISE simulations of merging galaxies a
Externí odkaz:
http://arxiv.org/abs/2102.02208
Autor:
Majewski, S. R., Forestell, A. D., Ostheimer, J. C., Palma, C., Siegel, M. H., Sohn, S., Westfall, K. B., Patterson, R. J., Frinchaboy, P. M., Link, R.
We are exploring the extended stellar distributions of Galactic satellite galaxies and globular clusters. For seven objects studied thus far, the observed profile departs from a King function at large r, revealing a ``break population'' of stars. In
Externí odkaz:
http://arxiv.org/abs/astro-ph/0109492
Autor:
Westfall, K. B., Andersen, D. R., Bershady, M. A., Martinsson, T. P. K., Swaters, R. A., Verheijen, M. A. W., Seigar, M.S., Treuthardt, P.
Publikováno v:
Structure and Dynamics of Disk Galaxies: Proceedings of the Conference held 12-16 August, 2013 at the Winthrop Rockefeller Institute, Petit Jean Mountain, Arkansas, USA, 480
We calculate the stellar surface mass density (Σ*) and two-component (gas+stars) disk stability (QRW) for 25 late-type galaxies from the DiskMass Survey. These calculations are based on fits of a dynamical model to our ionized-gas and stellar kinema
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::4df48675a2fa762032f6f51c9ad9bd06
https://research.rug.nl/en/publications/3b193ecb-5334-4a2c-9652-6935f3007051
https://research.rug.nl/en/publications/3b193ecb-5334-4a2c-9652-6935f3007051
Publikováno v:
Formation and Evolution of Galaxy Disks, 396
We analyze integral-field ionized gas and stellar line-of-sight kinematics in the context of determining the stellar velocity ellipsoid for spiral galaxies observed by the Disk-Mass Survey. Our new methodology enables us to measure, for the first tim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::176d017f59303f70042101cfeb5b1ed0
https://research.rug.nl/en/publications/5acfeb98-4da5-450c-a49d-edfe33161994
https://research.rug.nl/en/publications/5acfeb98-4da5-450c-a49d-edfe33161994
Publikováno v:
AIP Conference Proceedings; 2005, Vol. 752 Issue 1, p194-198, 5p
Autor:
Majewski, S. R., Forestell, A. D., Ostheimer, J. C., Palma, C., Siegel, M. H., Sohn, S., Westfall, K. B., Patterson, R. J., Frinchaboy, P. M., Link, R., Kunkel, W. E., Johnston, K. V.
Publikováno v:
Shapes of Galaxies & Their Dark Halos, the - Proceedings of the Yale Cosmology Workshop; 2002, p214-221, 8p
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