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Albedo, Size, and Surface Characteristics of Hayabusa-2 Sample-Return Target 162173 1999 JU3 from AKARI and Subaru Observations
Müller, T. G.; Wada, T.; Ita, Y. +7 more
Searching for mid-IR obscured AGN in the Chandra deep field North
Georgakakis, A.; Georgantopoulos, I.; Rovilos, E. +1 more
The efficiency of mid-infrared selection methods for finding obscured AGN is investigated using data in the Chandra Deep Field North. It is shown that samples of AGN candidates compiled on the basis of mid-infrared colours only suffer substantial contamination from normal galaxies. X-ray stacking analysis reveals a soft mean X-ray spectrum for the…
Suzaku Observation of the Ophiuchus Galaxy Cluster: One of the Hottest Cool Core Clusters
Sarazin, Craig L.; Reiprich, Thomas H.; Hayashida, Kiyoshi +6 more
We present the analysis of a Suzaku observation of the Ophiuchus galaxy cluster. We confirmed that the cluster has a cool core. While the temperature of the intracluster medium (ICM) decreases toward the center, the metal abundance increases. Except for the core (r lesssim 50kpc), the cluster is hot (∼9-10keV) and is almost isothermal for r lesssi…
Angular Diameters of the G Subdwarf µ Cassiopeiae A and the K Dwarfs σ Draconis and HR 511 from Interferometric Measurements with the CHARA Array
Gies, Douglas R.; Henry, Todd; Jao, Wei-Chun +13 more
Using the longest baselines of the CHARA Array, we have measured the angular diameter of the G5 V subdwarf µ Cas A, the first such determination for a halo population star. We compare this result to new diameters for the higher metallicity K0 V stars, σ Dra and HR 511, and find that the metal-poor star, µ Cas A, has an effective temper…
Star formation histories of early-type galaxies at z = 1.2 in cluster and field environments
Demarco, R.; Rosati, P.; Nonino, M. +3 more
We derive the star formation histories of early-type galaxies at z≃1.2 in both low and high density environments. To this purpose, we compare the co-added spectroscopic and 8-9 band photometric data of 43 mass selected early-type galaxies in the massive cluster RDCS J1252.9-2927 and the GOODS/CDF-S field with a large grid of composite stellar popu…
Sequestration of Ethane in the Cryovolcanic Subsurface of Titan
Mousis, Olivier; Schmitt, Bernard
Saturn's largest satellite, Titan, has a thick atmosphere dominated by nitrogen and methane. The dense orange-brown smog hiding the satellite's surface is produced by photochemical reactions of methane, nitrogen, and their dissociation products with solar ultraviolet, which lead primarily to the formation of ethane and heavier hydrocarbons. In the…
Auroral current systems in Saturn's magnetosphere: comparison of theoretical models with Cassini and HST observations
Coates, A. J.; Dougherty, M. K.; Nichols, J. D. +7 more
The first simultaneous observations of fields and plasmas in Saturn's high-latitude magnetosphere and UV images of the conjugate auroral oval were obtained by the Cassini spacecraft and the Hubble Space Telescope (HST) in January 2007. These data have shown that the southern auroral oval near noon maps to the dayside cusp boundary between open and…
Interferometric Detections of GOODS 850-5 at 1 mm and 1.4 GHz
Morrison, G.; Walter, F.; Dannerbauer, H.
We have obtained a position (at subarcsecond accuracy) of the submillimeter bright source GOODS 850-5 (also known as GN 10) in the GOODS-North field using the IRAM Plateau de Bure interferometer at 1.25 mm wavelengths (MM J123633+6214.1; flux density: S1.25 mm = 5.0 +/- 1.0 mJy). This source has no optical counterpart in deep ACS imagin…
Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud
Weigelt, G.; Hofmann, K. -H.; Driebe, T. +2 more
Aims: We present N-band spectro-interferometric observations of the red supergiant
The kinematic footprints of five stellar streams in Andromeda's halo
Tanvir, N.; Rich, R. M.; Koch, A. +12 more
We present a spectroscopic analysis of five stellar streams (`A', `B', `Cr', `Cp' and `D') as well as the extended star cluster, EC4, which lies within Stream`C', all discovered in the halo of M31 from our Canada-France-Hawaii Telescope/MegaCam survey. These spectroscopic results were initially serendipitous, making use of our existing observation…