Showing 2011Show all

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astro-ph.SR2011★ 74 cited

High resolution spectroscopy of Ne II emission from young stellar objects

G. G. Sacco, E. Flaccomio, I. Pascucci +6

Constraining the spatial and thermal structure of the gaseous component of circumstellar disks is crucial to understand star and planet formation. Models predict that the [Ne II] l…

astro-ph.GA2011★ 14 cited

Warm gas at 50 AU in the disk around Herbig Be star HD 100546

M. Goto, G. van der Plas, M. van den Ancker +6

The disk atmosphere is one of the fundamental elements of theoretical models of a protoplanetary disk. However, the direct observation of the warm gas (>> 100 K) at large radius of…

astro-ph.SR2011★ 13 cited

Finding proto-spectroscopic binaries: Precise multi-epoch radial velocities of 7 protostars in rho-Ophiuchus

P. Viana Almeida, C. Melo, N. C. Santos +3

The formation of spectroscopic binaries (SB) may be a natural byproduct of star formation. The early dynamical evolution of multiple stellar systems after the initial fragmentation…

astro-ph.CO2011★ 37 cited

Star Formation and AGN activity in Galaxies classified using the 1.6 μm Bump and PAH features at

Hitoshi Hanami, Tsuyoshi Ishigaki, Naofumi Fujishiro +17

We have studied the star-formation and AGN activity of massive galaxies in the redshift range , which are detected in a deep survey field using the AKARI InfraRed (IR) ast…

astro-ph.SR2011★ 7 cited

The narrow, inner CO ring around the magnetic Herbig Ae star, HD 101412

C. R. Cowley, S. Hubrig, F. Castelli +1

We describe and model emission lines in the first overtone band of CO in the magnetic Herbig Ae star HD 101412. High-resolution CRIRES spectra reveal unusually sharp features which…

astro-ph.SR2011★ 1 cited

Modeling the Asymmetric Wind of Massive LBV Binary MWC 314

A. Lobel, J. Groh, K. Torres Dozinel +13

Spectroscopic monitoring with Mercator-HERMES over the past two years reveals that MWC 314 is a massive binary system composed of an early B-type primary LBV star and a less-lumino…

astro-ph.EP2011★ 65 cited

Shape modeling technique KOALA validated by ESA Rosetta at (21) Lutetia

B. Carry, M. Kaasalainen, W. J. Merline +12

We present a comparison of our results from ground-based observations of asteroid (21) Lutetia with imaging data acquired during the flyby of the asteroid by the ESA Rosetta missio…

astro-ph.SR2011★ 8 cited

AMBER/VLTI observations of 5 giant stars

F. Cusano, C. Paladini, A. Richichi +6

While the search for exoplanets around main sequence stars more massive than the Sun have found relatively few such objects, surveys performed around giant stars have led to the di…

astro-ph.CO2011★ 18 cited

Spectroscopy of the spatially-extended Lya emission around a QSO at z=6.4

Tomotsugu Goto, Yousuke Utsumi, Jeremy R. Walsh +3

We have taken a deep, moderate-resolution Keck/Deimos spectra of QSO, CFHQS2329, at z=6.4. At the wavelength of Lya, the spectrum shows a spatially-extended component, which is sig…

astro-ph.CO2011★ 45 cited

Environmental effects in the interaction and merging of galaxies in zCOSMOS

P. Kampczyk, S. J. Lilly, L. de Ravel +56

(Abridged) We analyze the environments and galactic properties (morphologies and star-formation histories) of a sample of 153 close kinematic pairs in the redshift range 0.2 < z <…

astro-ph.CO2011★ 15 cited

A Magellan-IMACS-IFU Search for Dynamical Drivers of Nuclear Activity. I. Reduction Pipeline and Galaxy Catalog

Paul Westoby, Carole Mundell, Neil Nagar +5

Using the Inamori Magellan Areal Camera and Spectrograph (IMACS) integral-field unit (IFU) on the 6.5m Magellan telescope, we have designed the first statistically significant inve…

astro-ph.CO2011★ 76 cited

The specific frequencies of ultra-compact dwarf galaxies

Steffen Mieske, Michael Hilker, Ingo Misgeld

We aim at quantifying the specific frequency of UCDs in a range of environments and at relating this to the frequency of globular clusters (GCs) and potential progenitor dwarf gala…

astro-ph.CO2011★ 25 cited

The Cosmic Web and galaxy evolution around the most luminous X-ray cluster: RXJ1347.5-1145

M. Verdugo, M. Lerchster, H. Boehringer +5

In this paper we study the large scale structures and their galaxy content around the most X-ray luminous cluster known, RX J1347.5-1145 at z=0.45. We make use of ugriz CFHT MEGACA…

astro-ph.CO2011★ 113 cited

The ongoing assembly of a central cluster galaxy: Phase-space substructures in the halo of M87

Aaron J. Romanowsky, Jay Strader, Jean P. Brodie +5

The halos of galaxies preserve unique records of their formation histories. We carry out the first combined observational and theoretical study of phase-space halo substructure in…

astro-ph.GA2011★ 15 cited

Strengthening the Open Cluster Distance Scale via VVV Photometry

Daniel J. Majaess, David G. Turner, C. Moni Bidin +14

Approximately 14% of known Galactic open clusters possess absolute errors 20% as evaluated from n>3 independent distance estimates, and the statistics for age estimates are markedl…

astro-ph.CO2011★ 92 cited

The Atlas3D Project -- XI. Dense molecular gas properties of CO-luminous early-type galaxies

Alison Crocker, Melanie Krips, Martin Bureau +24

Surveying eighteen 12CO-bright galaxies from the ATLAS3D early-type galaxy sample with the Institut de Radio Astronomie Millimétrique (IRAM) 30m telescope, we detect 13CO(1-0) and…

astro-ph.GA2011★ 169 cited

More on the structure of tidal tails

Andreas H. W. Kuepper, Richard R. Lane, Douglas C. Heggie

We investigate the epicyclic motion of stars escaping from star clusters. Using streaklines, we visualise the path of escaping stars and show how epicyclic motion leads to over- an…

astro-ph.EP2011★ 51 cited

P/2010A2 LINEAR - I: An impact in the Asteroid Main Belt

O. R. Hainaut, J. Kleyna, G. Sarid +8

Comet P/2010A2 LINEAR is a good candidate for membership with the Main Belt Comet family. It was observed with several telescopes (ESO NTT, La Silla; Gemini North, Mauna Kea; UH 2.…

astro-ph.CO2011★ 37 cited

Do Nuclear Star Clusters and Black Holes Follow the Same Host-Galaxy Correlations?

Peter Erwin, Dimitri Gadotti

Studies have suggested that there is a strong correlation between the masses of nuclear star clusters (NSCs) and their host galaxies, a correlation which said to be an extension of…

astro-ph.EP2011★ 116 cited

EChO - Exoplanet Characterisation Observatory

G. Tinetti, J. P. Beaulieu, T. Henning +131

A dedicated mission to investigate exoplanetary atmospheres represents a major milestone in our quest to understand our place in the universe by placing our Solar System in context…

astro-ph.GA2011★ 3 cited

New Galactic Candidate Luminous Blue Variables and Wolf-Rayet Stars

Guy S. Stringfellow, Vasilii V. Gvaramadze, Yuri Beletsky +1

We have undertaken a near-infrared spectral survey of stars associated with compact mid-IR shells recently revealed by the MIPSGAL (24 micron) and GLIMPSE (8 micron) Spitzer survey…

astro-ph.EP2011★ 375 cited

Trapping dust particles in the outer regions of protoplanetary disks

P. Pinilla, T. Birnstiel, L. Ricci +4

In order to explain grain growth to mm sized particles and their retention in outer regions of protoplanetary disks, as it is observed at sub-mm and mm wavelengths, we investigate…

astro-ph.CO2011★ 336 cited

Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis (SIGMA)

Lee S. Kelvin, Simon P. Driver, Aaron S. G. Robotham +17

We present single-Sérsic two-dimensional model fits to 167,600 galaxies modelled independently in the ugrizYJHK bandpasses using reprocessed Sloan Digital Sky Survey Data Release S…

astro-ph.CO2011★ 226 cited

A Large Population of Massive Compact Post-Starburst Galaxies at z>1: Implications for the Size Evolution and Quenching Mechanism of Quiescent Galaxies

Katherine E. Whitaker, Mariska Kriek, Pieter G. van Dokkum +4

We study the growth of the red sequence through the number density and structural evolution of a sample of young and old quiescent galaxies at 0<z<2. The galaxies are selected from…