Search Publications

Witnessing galaxy assembly in an extended z≈3 structure
DOI: 10.1093/mnras/stx1896 Bibcode: 2017MNRAS.471.3686F

Prochaska, J. Xavier; Rafelski, Marc; Fumagalli, Michele +9 more

We present new observations acquired with the Multi Unit Spectroscopic Explorer instrument on the Very Large Telescope in a quasar field that hosts a high column density damped Lyα absorber (DLA) at z ≈ 3.25. We detect Lyα emission from a nebula at the redshift of the DLA with line luminosity (27 ± 1) × 1041 erg s- 1, which e…

2017 Monthly Notices of the Royal Astronomical Society
eHST 49
Detection of the Ultraviolet Spectrum of the Hot Subdwarf Companion of 60 Cygni (B1 Ve) from a Survey of IUE Spectra of Be Stars
DOI: 10.3847/1538-4357/aa740a Bibcode: 2017ApJ...843...60W

Gies, Douglas R.; Wang, Luqian; Peters, Geraldine J.

We used archival International Ultraviolet Explorer (IUE) high-dispersion, short wavelength spectra data to search for evidence of the spectra of hot subdwarf companions of six rapidly rotating Be stars in binary systems. We searched for the signature of a hot companion through an analysis of the cross-correlation functions (CCFs) of observed and …

2017 The Astrophysical Journal
Gaia IUE 49
The relationship between star formation activity and galaxy structural properties in CANDELS and a semi-analytic model
DOI: 10.1093/mnras/stw2690 Bibcode: 2017MNRAS.465..619B

Barro, Guillermo; Bell, Eric F.; Ferguson, Henry C. +13 more

We study the correlation of galaxy structural properties with their location relative to the SFR-M* correlation, also known as the star formation `star-forming main sequence' (SFMS), in the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey and Galaxy and Mass Assembly Survey and in a semi-analytic model (SAM) of galaxy form…

2017 Monthly Notices of the Royal Astronomical Society
eHST 49
The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles: The Largest Herschel Survey of the Extragalactic Sky
DOI: 10.3847/1538-4365/aa9b35 Bibcode: 2017ApJS..233...26S

Smith, Matthew W. L.; Dunne, Loretta; Viaene, Sébastien +11 more

We present the largest submillimeter images that have been made of the extragalactic sky. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg2 with the PACS and SPIRE cameras in five photometric bands: 100, 160, 250, 350, and 500 µm. In this paper we present the images from our two largest field…

2017 The Astrophysical Journal Supplement Series
Herschel Planck 49
Fermi Non-detections of Four X-Ray Jet Sources and Implications for the IC/CMB Mechanism
DOI: 10.3847/1538-4357/aa907a Bibcode: 2017ApJ...849...95B

Georganopoulos, Markos; Breiding, Peter; Meyer, Eileen T. +3 more

Since its launch in 1999, the Chandra X-ray observatory has discovered several dozen X-ray jets associated with powerful quasars. In many cases, the X-ray spectrum is hard and appears to come from a second spectral component. The most popular explanation for the kpc-scale X-ray emission in these cases has been inverse-Compton (IC) scattering of Co…

2017 The Astrophysical Journal
eHST 48
Properties of Turbulence in the Reconnection Exhaust: Numerical Simulations Compared with Observations
DOI: 10.3847/1538-4357/aa704f Bibcode: 2017ApJ...841...60P

Sorriso-Valvo, L.; Goldman, M. V.; Newman, D. L. +6 more

The properties of the turbulence that develops in the outflows of magnetic reconnection have been investigated using self-consistent plasma simulations, in three dimensions. As commonly observed in space plasmas, magnetic reconnection is characterized by the presence of turbulence. Here we provide a direct comparison of our simulations with report…

2017 The Astrophysical Journal
Cluster 48
SPHERE/ZIMPOL observations of the symbiotic system R Aquarii. I. Imaging of the stellar binary and the innermost jet clouds
DOI: 10.1051/0004-6361/201629416 Bibcode: 2017A&A...602A..53S

Quanz, S. P.; Siebenmorgen, R.; Stute, M. +40 more

Context. R Aqr is a symbiotic binary system consisting of a mira variable, a hot companion with a spectacular jet outflow, and an extended emission line nebula. Because of its proximity to the Sun, this object has been studied in much detail with many types of high resolution imaging and interferometric techniques. We have used R Aqr as test targe…

2017 Astronomy and Astrophysics
eHST 48
Suprathermal electron acceleration in the near-Earth flow rebounce region
DOI: 10.1002/2016JA023437 Bibcode: 2017JGRA..122..594L

Cao, J. B.; Xu, Y.; Yao, Z. H. +4 more

Flux pileup regions (FPRs) are traditionally referred to the strong-Bz bundles behind dipolarization fronts (DFs) in the Earth's magnetotail and can appear both inside earthward and tailward bursty bulk flows. It has been widely reported that suprathermal electrons (40-200 keV) can be efficiently accelerated inside earthward FPRs, leavi…

2017 Journal of Geophysical Research (Space Physics)
Cluster 48
Observational Evidence for the Associated Formation of Blobs and Raining Inflows in the Solar Corona
DOI: 10.3847/2041-8213/835/1/L7 Bibcode: 2017ApJ...835L...7S

Davies, J. A.; Lavraud, B.; Kilpua, E. +6 more

The origin of the slow solar wind is still a topic of much debate. The continual emergence of small transient structures from helmet streamers is thought to constitute one of the main sources of the slow wind. Determining the height at which these transients are released is an important factor in determining the conditions under which the slow sol…

2017 The Astrophysical Journal
SOHO 48
H2CO Distribution and Formation in the TW HYA Disk
DOI: 10.3847/1538-4357/aa689a Bibcode: 2017ApJ...839...43O

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +8 more

H2CO is one of the most readily detected organic molecules in protoplanetary disks. Yet its distribution and dominant formation pathway(s) remain largely unconstrained. To address these issues, we present ALMA observations of two H2CO lines ({3}12{--}{2}11 and {5}15{--}{4}14) at 0.″…

2017 The Astrophysical Journal
Gaia 48