Search Publications

The Ionized Gas in Nearby Galaxies as Traced by the [N II] 122 and 205 µm Transitions
DOI: 10.3847/0004-637X/826/2/175 Bibcode: 2016ApJ...826..175H

Boquien, M.; Rigopoulou, D.; Armus, L. +20 more

The [N II] 122 and 205 µm transitions are powerful tracers of the ionized gas in the interstellar medium. By combining data from 21 galaxies selected from the Herschel KINGFISH and Beyond the Peak surveys, we have compiled 141 spatially resolved regions with a typical size of ∼1 kpc, with observations of both [N II] far-infrared lines. We me…

2016 The Astrophysical Journal
Herschel 64
Hα features with hot onsets. I. Ellerman bombs
DOI: 10.1051/0004-6361/201526489 Bibcode: 2016A&A...590A.124R

Rutten, R. J.

Ellerman bombs are transient brightenings of the wings of the Balmer lines that uniquely mark reconnection in the solar photosphere. They are also bright in strong Ca II and ultraviolet lines and in ultraviolet continua, but they are not visible in the optical continuum and the Na I D and Mg I b lines. These discordant visibilities invalidate all …

2016 Astronomy and Astrophysics
IRIS 63
Refining the Dynamical Clock for Star Clusters
DOI: 10.3847/2041-8213/833/2/L29 Bibcode: 2016ApJ...833L..29L

Dalessandro, E.; Vesperini, E.; Ferraro, F. R. +3 more

We used a sample of 25 Galactic globular clusters to empirically measure the parameter A + recently introduced by Alessandrini et al., and defined as the area enclosed between the cumulative radial distribution of blue straggler stars (BSSs) and that of a reference population. Based on N-body simulations, this parameter is expected to e…

2016 The Astrophysical Journal
eHST 63
Orbital and physical characteristics of meter-scale impactors from airburst observations
DOI: 10.1016/j.icarus.2015.11.022 Bibcode: 2016Icar..266...96B

Brown, P.; Clark, D.; Wiegert, P. +1 more

We have analyzed the orbits and ablation characteristics in the atmosphere of 59 Earth-impacting fireballs, produced by meteoroids 1 m in diameter or larger, described here as meter-scale. Using heights at peak luminosity as a proxy for strength, we determine that there is roughly an order of magnitude spread in strengths of the population of mete…

2016 Icarus
VenusExpress 63
Planck intermediate results. XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
DOI: 10.1051/0004-6361/201628636 Bibcode: 2016A&A...596A.105P

Miville-Deschênes, M. -A.; Boulanger, F.; Bernard, J. -P. +165 more

Using data from the Planck satellite, we study the statistical properties of interstellar dust polarization at high Galactic latitudes around the south pole (b < -60°). Our aim is to advance the understanding of the magnetized interstellar medium (ISM), and to provide a modelling framework of the polarized dust foreground for use in cosmic micr…

2016 Astronomy and Astrophysics
Planck 63
Cosmological constraints on decoupled dark photons and dark Higgs
DOI: 10.1088/1475-7516/2016/11/032 Bibcode: 2016JCAP...11..032B

Berger, Joshua; Jedamzik, Karsten; Walker, Devin G. E.

Any neutral boson such as a dark photon or dark Higgs that is part of a non-standard sector of particles can mix with its standard model counterpart. When very weakly mixed with the Standard Model, these particles are produced in the early Universe via the freeze-in mechanism and subsequently decay back to standard model particles. In this work, w…

2016 Journal of Cosmology and Astroparticle Physics
Planck 63
Dark matter component decaying after recombination: Lensing constraints with Planck data
DOI: 10.1103/PhysRevD.94.023528 Bibcode: 2016PhRvD..94b3528C

Chudaykin, A.; Gorbunov, D.; Tkachev, I.

It has been recently suggested [Z. Berezhiani, A. D. Dolgov, and I. I. Tkachev, Phys. Rev. D 92, 061303 (2015)] that emerging tension between cosmological parameter values derived in high-redshift (CMB anisotropy) and low-redshift (cluster counts, Hubble constant) measurements can be reconciled in a model which contains a subdominant fraction of d…

2016 Physical Review D
Planck 63
Dust attenuation in z ~ 1 galaxies from Herschel and 3D-HST Hα measurements
DOI: 10.1051/0004-6361/201526782 Bibcode: 2016A&A...586A..83P

Berta, S.; Lutz, D.; Cimatti, A. +12 more

We combined the spectroscopic information from the 3D-HST survey with Herschel data to characterize the Hα dust attenuation properties of a sample of 79 main sequence star-forming galaxies at z ~ 1 in the GOODS-S field. The sample was selected in the far-IR at λ = 100 and/or 160 µm and only includes galaxies with a secure Hα detection (S/N &…

2016 Astronomy and Astrophysics
Herschel eHST 63
Reconnection brightenings in the quiet solar photosphere
DOI: 10.1051/0004-6361/201628889 Bibcode: 2016A&A...592A.100R

Rouppe van der Voort, Luc H. M.; Rutten, Robert J.; Vissers, Gregal J. M.

We describe a new quiet-Sun phenomenon which we call quiet-Sun Ellerman-like brightenings (QSEB). QSEBs are similar to Ellerman bombs (EB) in some respects but differ significantly in others. EBs are transient brightenings of the wings of the Balmer Hα line that mark strong-field photospheric reconnection in complex active regions. QSEBs are simil…

2016 Astronomy and Astrophysics
IRIS 63
Gamma rays detected from Cygnus X-1 with likely jet origin
DOI: 10.1051/0004-6361/201628917 Bibcode: 2016A&A...596A..55Z

Aharonian, F.; Blanch, O.; de Oña Wilhelmi, E. +4 more


Aims: We probe the high-energy (>60 MeV) emission from the black hole X-ray binary system, Cygnus X-1, and investigate its origin.
Methods: We analyzed 7.5 yr of data by Fermi-LAT with the latest Pass 8 software version.
Results: We report the detection of a signal at 8σ statistical significance that is spatially coincident with …

2016 Astronomy and Astrophysics
INTEGRAL 63