Search Publications

The selective effect of environment on the atomic and molecular gas-to-dust ratio of nearby galaxies in the Herschel Reference Survey
DOI: 10.1093/mnras/stw801 Bibcode: 2016MNRAS.459.3574C

Ciesla, L.; Boquien, M.; Baes, M. +10 more

We combine dust, atomic (H I) and molecular (H2) hydrogen mass measurements for 176 galaxies in the Herschel Reference Survey to investigate the effect of environment on the gas-to-dust mass (Mgas/Mdust) ratio of nearby galaxies. We find that, at fixed stellar mass, the average Mgas/Mdust rati…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 46
Parallax and masses of α Centauri revisited
DOI: 10.1051/0004-6361/201527859 Bibcode: 2016A&A...586A..90P

Boffin, Henri M. J.; Pourbaix, Dimitri

Context. Despite the thorough work of van Leeuwen, the parallax of α Centauri is still far from being carved in stone. Any derivation of the individual masses is therefore uncertain, if not questionable. And yet, that does not prevent this system from being used for calibration purpose in several studies.
Aims: We aim for more accurate model-…

2016 Astronomy and Astrophysics
Hipparcos 46
A statistical study of EMIC waves observed by Cluster: 2. Associated plasma conditions
DOI: 10.1002/2016JA022541 Bibcode: 2016JGRA..121.6458A

André, M.; Klecker, B.; Kistler, L. M. +6 more

This is the second in a pair of papers discussing a statistical study of electromagnetic ion cyclotron (EMIC) waves detected during 10 years (2001-2010) of Cluster observations. In the first paper, an analysis of EMIC wave properties (i.e., wave power, polarization, normal angle, and wave propagation angle) is presented in both the magnetic latitu…

2016 Journal of Geophysical Research (Space Physics)
Cluster 46
What Is Controlling the Fragmentation in the Infrared Dark Cloud G14.225-0.506?: Different Levels of Fragmentation in Twin Hubs.
DOI: 10.3847/0004-637X/819/2/139 Bibcode: 2016ApJ...819..139B

Zhang, Qizhou; Palau, Aina; Pillai, Thushara +7 more

We present observations of the 1.3 mm continuum emission toward hub-N and hub-S of the infrared dark cloud G14.225-0.506 carried out with the Submillimeter Array, together with observations of the dust emission at 870 and 350 µm obtained with APEX and CSO telescopes. The large-scale dust emission of both hubs consists of a single peaked clum…

2016 The Astrophysical Journal
Herschel 46
Quasi-periodic Pulsations during the Impulsive and Decay phases of an X-class Flare
DOI: 10.3847/2041-8205/827/2/L30 Bibcode: 2016ApJ...827L..30H

Hayes, L. A.; Gallagher, P. T.; Dennis, B. R. +3 more

Quasi-periodic pulsations (QPPs) are often observed in X-ray emission from solar flares. To date, it is unclear what their physical origins are. Here, we present a multi-instrument investigation of the nature of QPP during the impulsive and decay phases of the X1.0 flare of 2013 October 28. We focus on the character of the fine structure pulsation…

2016 The Astrophysical Journal
PROBA-2 46
The Infrared Spectral Properties of Magellanic Carbon Stars
DOI: 10.3847/0004-637X/826/1/44 Bibcode: 2016ApJ...826...44S

van Loon, J. Th.; Sahai, R.; Wood, P. R. +12 more

The Infrared Spectrograph on the Spitzer Space Telescope observed 184 carbon stars in the Magellanic Clouds. This sample reveals that the dust-production rate (DPR) from carbon stars generally increases with the pulsation period of the star. The composition of the dust grains follows two condensation sequences, with more SiC condensing before amor…

2016 The Astrophysical Journal
ISO 46
The near-to-mid infrared spectrum of quasars
DOI: 10.1093/mnras/stw2107 Bibcode: 2016MNRAS.463.2064H

Alonso-Herrero, Almudena; Hatziminaoglou, Evanthia; Hernán-Caballero, Antonio +1 more

We analyse a sample of 85 luminous (log (νLν(3 µm)/erg s-1) > 45.5) quasars with rest frame ∼2-11 µm spectroscopy from AKARI and Spitzer. Their high luminosity allows a direct determination of the near-infrared quasar spectrum free from host galaxy emission. A semi-empirical model consisting of a single templat…

2016 Monthly Notices of the Royal Astronomical Society
AKARI 46
A Deep Campaign to Characterize the Synchronous Radio/X-Ray Mode Switching of PSR B0943+10
DOI: 10.3847/0004-637X/831/1/21 Bibcode: 2016ApJ...831...21M

Tiengo, A.; Mereghetti, S.; Esposito, P. +14 more

Observations of PSR B0943+10 with XMM-Newton and the LOFAR, LWA, and Arecibo radio telescopes in 2014 November confirm the synchronous X-ray/radio switching between a radio-bright (B) mode and a radio-quiet (Q) mode, in which the X-ray flux is a factor ∼2.4 higher than in the B-mode. We discovered X-ray pulsations during the B-mode (0.5-2 keV puls…

2016 The Astrophysical Journal
XMM-Newton 46
Low Gas Fractions Connect Compact Star-forming Galaxies to Their z ~ 2 Quiescent Descendants
DOI: 10.3847/0004-637X/832/1/19 Bibcode: 2016ApJ...832...19S

Weiner, Benjamin J.; Bezanson, Rachel; Williams, Christina C. +3 more

Early quiescent galaxies at z∼ 2 are known to be remarkably compact compared to their nearby counterparts. Possible progenitors of these systems include galaxies that are structurally similar, but are still rapidly forming stars. Here, we present Karl G. Jansky Very Large Array (VLA) observations of the CO(1-0) line toward three such compact, star…

2016 The Astrophysical Journal
eHST 46
Absorption-line Spectroscopy of Gravitationally Lensed Galaxies: Further Constraints on the Escape Fraction of Ionizing Photons at High Redshift
DOI: 10.3847/0004-637X/831/2/152 Bibcode: 2016ApJ...831..152L

Stark, Daniel P.; Ellis, Richard S.; Zitrin, Adi +2 more

The fraction of ionizing photons escaping from high-redshift star-forming galaxies is a key obstacle in evaluating whether galaxies were the primary agents of cosmic reionization. We previously proposed using the covering fraction of low-ionization gas, measured via deep absorption-line spectroscopy, as a proxy. We now present a significant update…

2016 The Astrophysical Journal
eHST 46