Search Publications

Variations in cometary dust composition from Giotto to Rosetta, clues to their formation mechanisms
DOI: 10.1093/mnras/stw2844 Bibcode: 2016MNRAS.462S.323E

Langevin, Yves; Fischer, Henning; Briois, Christelle +18 more

This paper reviews the current knowledge on the composition of cometary dust (ice, minerals and organics) in order to constrain their origin and formation mechanisms. Comets have been investigated by astronomical observations, space missions (Giotto to Rosetta), and by the analysis of cometary dust particles collected on Earth, chondritic porous i…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta 21
Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution since z = 1.6
DOI: 10.1051/0004-6361/201526563 Bibcode: 2016A&A...592A.132G

Gargiulo, A.; Saracco, P.; Tamburri, S. +2 more


Aims: We investigate the stellar mass assembly history of ultramassive (M ≳ 1011M) dense (Σ = M/2πRe2> 2500M pc-2) early-type galaxies (ETGs, elliptical and spheroidal galaxies) selected on basis of visual classification over the last 9 Gyr.
Me…

2016 Astronomy and Astrophysics
eHST 21
A Search for Hyperluminous X-Ray Sources in the XMM-Newton Source Catalog
DOI: 10.3847/0004-637X/817/2/88 Bibcode: 2016ApJ...817...88Z

Bachetti, M.; Godet, O.; Webb, N. A. +2 more

We present a new method to identify luminous off-nuclear X-ray sources in the outskirts of galaxies from large public redshift surveys, distinguishing them from foreground and background interlopers. Using the 3XMM-DR5 catalog of X-ray sources and the SDSS DR12 spectroscopic sample of galaxies, with the help of this off-nuclear cross-matching tech…

2016 The Astrophysical Journal
XMM-Newton 21
Chandra X-Ray and Hubble Space Telescope Imaging of Optically Selected Kiloparsec-scale Binary Active Galactic Nuclei. II. Host Galaxy Morphology and AGN Activity
DOI: 10.3847/0004-637X/823/1/50 Bibcode: 2016ApJ...823...50S

Shen, Yue; Ho, Luis C.; Strauss, Michael A. +4 more

Binary active galactic nuclei (AGNs) provide clues to how gas-rich mergers trigger and fuel AGNs and how supermassive black hole (SMBH) pairs evolve in a gas-rich environment. While significant effort has been invested in their identification, the detailed properties of binary AGNs and their host galaxies are still poorly constrained. In a compani…

2016 The Astrophysical Journal
eHST 21
Systematic or signal? How dark matter misalignments can bias strong lensing models of galaxy clusters
DOI: 10.1093/mnras/stw295 Bibcode: 2016MNRAS.458..660H

Kneib, J. P.; Jauzac, M.; Harvey, D.

We explore how assuming that mass traces light in strong gravitational lensing models can lead to systematic errors in the predicted position of multiple images. Using a model based on the galaxy cluster MACS J0416 (z = 0.397) from the Hubble Frontier Fields, we split each galactic halo into a baryonic and dark matter component. We then shift the …

2016 Monthly Notices of the Royal Astronomical Society
eHST 21
Improved algorithm for the transmittance estimation of spectra obtained with SOIR/Venus Express
DOI: 10.1364/AO.55.009275 Bibcode: 2016ApOpt..55.9275T

Bertaux, Jean-Loup; Vandaele, Ann Carine; Ristic, Bojan +5 more

2016 Applied Optics
VenusExpress 21
Controlling Influence of Magnetic Field on Solar Wind Outflow: An Investigation using Current Sheet Source Surface Model
DOI: 10.3847/2041-8205/827/1/L6 Bibcode: 2016ApJ...827L...6P

Poduval, B.

This Letter presents the results of an investigation into the controlling influence of large-scale magnetic field of the Sun in determining the solar wind outflow using two magnetostatic coronal models: current sheet source surface (CSSS) and potential field source surface. For this, we made use of the Wang and Sheeley inverse correlation between …

2016 The Astrophysical Journal
SOHO 21
Resolving the Fan-spine Reconnection Geometry of a Small-scale Chromospheric Jet Event with the New Solar Telescope
DOI: 10.3847/2041-8205/819/1/L3 Bibcode: 2016ApJ...819L...3Z

Chen, Bin; Cao, Wenda; Goode, Philip R. +2 more

Jets are ubiquitously present in both quiet and active regions on the Sun. They are widely believed to be driven by magnetic reconnection. A fan-spine structure has been frequently reported in some coronal jets and flares, and has been regarded as a signature of ongoing magnetic reconnection in a topology consisting of a magnetic null connected by…

2016 The Astrophysical Journal
Hinode 21
SOAR Optical and Near-infrared Spectroscopic Survey of Newly Discovered Massive Stars in the Periphery of Galactic Massive Star Clusters I-NGC 3603
DOI: 10.3847/0004-637X/823/2/96 Bibcode: 2016ApJ...823...96R

Roman-Lopes, A.; Sanmartim, D.; Franco, G. A. P.

In this work, we present the results of a spectroscopic study of very massive stars (VMSs) found outside the center of the massive stellar cluster NGC 3603. From the analysis of the associated Southern Astrophysical Research (SOAR) Telescope spectroscopic data and related optical-near-IR (NIR) photometry, we confirm the existence of several VMSs i…

2016 The Astrophysical Journal
XMM-Newton 21
3C 279 in Outburst in 2015 June: A Broadband SED Study Based on the INTEGRAL Detection
DOI: 10.3847/0004-637X/832/1/17 Bibcode: 2016ApJ...832...17B

Pian, Elena; Böttcher, Markus; Bottacini, Eugenio +1 more

Blazars radiate from radio through gamma-ray frequencies and thereby make ideal targets for multifrequency studies. Such studies allow the properties of the emitting jet to be constrained. 3C 279 is among the most notable blazars and therefore subject to extensive multifrequency campaigns. We report the results of a campaign ranging from near-IR t…

2016 The Astrophysical Journal
INTEGRAL 21