The cometary activity very far from the Sun: the case of C/2007 D1 (LINEAR) and other stories of comets
Not Available
Mazzotta Epifani, E. et al.
Advertised on:
9
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/
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The Chemical Evolution of the Monoceros Ring/Galactic Anticenter Stellar StructureThe origin of the Galactic Anticenter Stellar Structure (GASS) or "Monoceros Ring"—a low-latitude overdensity at the edge of the Galactic disk spanning at least the second and third Galactic quadrants—remains controversial. Models for the origin of GASS generally fall into scenarios where either it is a part (e.g., warp) of the Galactic disk or itChou, Mei-Yin et al.
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92010 -
The Afterglows of Swift-era Gamma-ray Bursts. I. Comparing pre-Swift and Swift-era Long/Soft (Type II) GRB Optical AfterglowsWe have gathered optical photometry data from the literature on a large sample of Swift-era gamma-ray burst (GRB) afterglows including GRBs up to 2009 September, for a total of 76 GRBs, and present an additional three pre-Swift GRBs not included in an earlier sample. Furthermore, we publish 840 additional new photometry data points on a total of 42Kann, D. A. et al.
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92010 -
The ACS LCID Project. III. The Star Formation History of the Cetus dSph Galaxy: A Post-reionization FossilWe use deep HST/ACS observations to calculate the star formation history (SFH) of the Cetus dwarf spheroidal (dSph) galaxy. Our photometry reaches below the oldest main-sequence turnoffs, which allows us to estimate the age and duration of the main episode of star formation in Cetus. This is well approximated by a single episode that peaked roughlyMonelli, M. et al.
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92010 -
Superdense Massive Galaxies in the ESO Distant Cluster Survey (EDisCS)We find a significant number of massive and compact galaxies in clusters from the ESO Distant Clusters Survey (EDisCS) at 0.4 z 1. They have similar stellar masses, ages, sizes, and axial ratios to local z ~ 0.04 compact galaxies in WIde field Nearby Galaxy clusters Survey (WINGS) clusters, and to z = 1.4-2 massive and passive galaxies found inValentinuzzi, T. et al.
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92010 -
Study of the oxygen day glow in the Martian atmosphere with nadir data of PFS-MEXNot AvailableGeminale, A. et al.
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92010