Search Publications

Starbursts and dusty tori in distant 3CR radio galaxies
DOI: 10.1093/mnras/stw1946 Bibcode: 2016MNRAS.462.4183P

Barthel, Peter; Drouart, Guillaume; Podigachoski, Pece +2 more

We present a study of the complete ultraviolet to submillimetre spectral energy distributions (SEDs) of 12 3CR radio galaxy hosts in the redshift range 1.0 < z < 2.5, which were all detected in the far-infrared by the Herschel Space Observatory. The study employs the new spectro-chemical evolutionary code PÉGASE.3, in combination with recent…

2016 Monthly Notices of the Royal Astronomical Society
Herschel eHST 17
The Tale of the Two Tails of the Oldish PSR J2055+2539
DOI: 10.3847/0004-637X/819/1/40 Bibcode: 2016ApJ...819...40M

De Luca, Andrea; Caraveo, Patrizia; Marelli, Martino +3 more

We analyzed a deep XMM-Newton observation of the radio-quiet γ-ray PSR J2055+2539. The spectrum of the X-ray counterpart is nonthermal, with a photon index of Γ = 2.36 ± 0.14 (1σ confidence). We detected X-ray pulsations with a pulsed fraction of 25% ± 3% and a sinusoidal shape. Taking into account considerations on the γ-ray efficiency of the pul…

2016 The Astrophysical Journal
XMM-Newton 17
Genesis of Interplanetary Intermittent Turbulence: A Case Study of Rope&enrope Magnetic Reconnection
DOI: 10.3847/0004-637X/832/2/179 Bibcode: 2016ApJ...832..179C

Miranda, Rodrigo A.; Chian, Abraham C. -L.; Muñoz, Pablo R. +5 more

In a recent paper, the relation between current sheet, magnetic reconnection, and turbulence at the leading edge of an interplanetary coronal mass ejection was studied. We report here the observation of magnetic reconnection at the interface region of two interplanetary magnetic flux ropes. The front and rear boundary layers of three interplanetar…

2016 The Astrophysical Journal
Cluster 17
Dipole modulation of cosmic microwave background temperature and polarization
DOI: 10.1088/1475-7516/2016/01/046 Bibcode: 2016JCAP...01..046G

Ghosh, Shamik; Kothari, Rahul; Jain, Pankaj +1 more

We propose a dipole modulation model for the Cosmic Microwave Background Radiation (CMBR) polarization field. We show that the model leads to correlations between l and l+1 multipoles, exactly as in the case of temperature. We obtain results for the case of TE, EE and BB correlations. An anisotropic or inhomogeneous model of primordial power spect…

2016 Journal of Cosmology and Astroparticle Physics
Planck 17
Searching for filaments and large-scale structure around DAFT/FADA clusters
DOI: 10.1051/0004-6361/201527655 Bibcode: 2016A&A...588A..69D

Adami, C.; Martinet, N.; Durret, F. +6 more

Context. Clusters of galaxies are located at the intersection of cosmic filaments and are still accreting galaxies and groups along these preferential directions. However, because of their relatively low contrast on the sky, filaments are difficult to detect (unless a large amount of spectroscopic data are available), and unambiguous detections ha…

2016 Astronomy and Astrophysics
eHST 17
The First High-phase Observations of a KBO: New Horizons Imaging of (15810) 1994 JR1 from the Kuiper Belt
DOI: 10.3847/2041-8205/828/2/L15 Bibcode: 2016ApJ...828L..15P

Olkin, Cathy B.; Stern, S. Alan; Young, Leslie A. +12 more

NASA’s New Horizons spacecraft observed (15810) 1994 JR1, a 3:2 resonant Kuiper belt object (KBO), using the LOng Range Reconnaissance Imager (LORRI) on 2015 November 2 from a distance of 1.85 au and again on 2016 April 7 from a distance of 0.71 au. These were the first close observations of any KBO other than Pluto. Combining ground-ba…

2016 The Astrophysical Journal
eHST 16
Probing the statistical properties of CMB B-mode polarization through Minkowski functionals
DOI: 10.1088/1475-7516/2016/07/029 Bibcode: 2016JCAP...07..029S

Wang, Kai; Santos, Larissa; Zhao, Wen

The detection of the magnetic type B-mode polarization is the main goal of future cosmic microwave background (CMB) experiments. In the standard model, the B-mode map is a strong non-gaussian field due to the CMB lensing component. Besides the two-point correlation function, the other statistics are also very important to dig the information of th…

2016 Journal of Cosmology and Astroparticle Physics
Planck 16
High spatial resolution optical imaging of the multiple T Tauri system Lk Hα 262/Lk Hα 263
DOI: 10.1093/mnras/stw1071 Bibcode: 2016MNRAS.460.3519V

Rebolo, R.; Labadie, L.; Velasco, S. +12 more

We report high spatial resolution I' band imaging of the multiple T Tauri system LkHα 262/LkHα 263 obtained during the first commissioning period of the Adaptive Optics Lucky Imager (AOLI) at the 4.2-m William Herschel Telescope, using its Lucky Imaging mode. AOLI images have provided photometry for each of the two components LkHα 263 A and B (0.4…

2016 Monthly Notices of the Royal Astronomical Society
eHST 16
Survival of Pure Disk Galaxies over the Last 8 Billion Years
DOI: 10.3847/2041-8205/820/1/L4 Bibcode: 2016ApJ...820L...4S

Sachdeva, Sonali; Saha, Kanak

Pure disk galaxies without any bulge component, I.e., bulges that are neither classical nor pseudo, seem to have escaped the effects of merger activity that are inherent to hierarchical galaxy formation models as well as strong internal secular evolution. We discover that a significant fraction (∼15%-18%) of disk galaxies in the Hubble Deep Field …

2016 The Astrophysical Journal
eHST 16
AKARI/IRC Near-infrared Spectral Atlas of Galactic Planetary Nebulae
DOI: 10.3847/0004-6256/151/4/93 Bibcode: 2016AJ....151...93O

Onaka, Takashi; Matsuura, Mikako; Sakon, Itsuki +2 more

Near-infrared (2.5-5.0 µm) low-resolution (λ/Δλ ∼ 100) spectra of 72 Galactic planetary nebulae (PNe) were obtained with the Infrared Camera (IRC) in the post-helium phase. The IRC, equipped with a 1‧ × 1‧ window for spectroscopy of a point source, was capable of obtaining near-infrared spectra in a slit-less mode without any flux loss due t…

2016 The Astronomical Journal
AKARI 16