Minor Planet Observations [511 Haute Provence]
Not Available
Arlot, J. E. et al.
Advertised on:
4
2010
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
-
-
Minor Planet Observations [304 Las Campanas Observatory]Not AvailableBenecchi, S. et al.
Advertised on:
42010 -
MILES SSP ModelsWe present SEDs for single-age, single-metallicity stellar populations (SSPs) covering the full optical spectral range at resolution (FWHM = 2.3Å). These SEDs can be regarded as our base models, as we combine scaled-solar isochrones with an empirical stellar spectral library (MILES), which follows the chemical evolution pattern of the solarVazdekis, A. et al.
Advertised on:
42010 -
Mild Velocity Dispersion Evolution of massive galaxies since z~2Making use of public spectra from Cimatti et al. (2008), we measure for the first time the velocity dispersion of spheroid-like massive (M* ~ 1011M&sun;) galaxies at z ~ 1.6. By comparing with galaxies of similar stellar mass at lower redshifts, we find evidence for a mild evolution in velocity dispersion, decreasing from ~240 kms-1 at z ~ 1.6 downTrujillo, I. et al.
Advertised on:
42010 -
Microbial Communities that are Concealed Within Mineral Deposits: Expanding our Detection of LifeIn addition to clearly biological microbial mats, lava tubes contain many non-biological appearing mineral deposits that contain life. The discovery that such deposits contain abundant life can help guide our detection of life on other extrater-restrial bodies.Northup, D. E. et al.
Advertised on:
42010 -
Metallicity gradients in dwarf elliptical galaxiesWe discuss the relations between the metallicity gradients and the other characteristics of a set of dwarf elliptical galaxies in different environments. We suggest that dEs have typically metallicity gradients of -0.30 ± 0.25 dex/re, unrelated to their mass. Dwarf elliptical galaxies with embedded disks, or dS0, may have flat metallicity gradientsKoleva, M. et al.
Advertised on:
42010