Search Publications

Sulphur monoxide exposes a potential molecular disk wind from the planet-hosting disk around HD 100546
DOI: 10.1051/0004-6361/201731347 Bibcode: 2018A&A...611A..16B

Booth, Alice S.; Walsh, Catherine; Loomis, Ryan A. +3 more

Sulphur-bearing volatiles are observed to be significantly depleted in interstellar and circumstellar regions. This missing sulphur is postulated to be mostly locked up in refractory form. With ALMA we have detected sulphur monoxide (SO), a known shock tracer, in the HD 100546 protoplanetary disk. Two rotational transitions: J = 77-6

2018 Astronomy and Astrophysics
Gaia 39
Measuring impact crater depth throughout the solar system
DOI: 10.1111/maps.12956 Bibcode: 2018M&PS...53..583R

Beyer, Ross A.; Robbins, Stuart J.; Watters, Wesley A. +9 more

One important, almost ubiquitous, tool for understanding the surfaces of solid bodies throughout the solar system is the study of impact craters. While measuring a distribution of crater diameters and locations is an important tool for a wide variety of studies, so too is measuring a crater's "depth." Depth can inform numerous studies including th…

2018 Meteoritics and Planetary Science
MEx 39
Revolutionizing Our Understanding of AGN Feedback and its Importance to Galaxy Evolution in the Era of the Next Generation Very Large Array
DOI: 10.3847/1538-4357/aab3d1 Bibcode: 2018ApJ...859...23N

Prandoni, I.; Rujopakarn, W.; Murphy, E. J. +19 more

Energetic feedback by active galactic nuclei (AGNs) plays an important evolutionary role in the regulation of star formation on galactic scales. However, the effects of this feedback as a function of redshift and galaxy properties such as mass, environment, and cold gas content remain poorly understood. The broad frequency coverage (1 to 116 GHz),…

2018 The Astrophysical Journal
eHST 39
X-ray study of the double radio relic Abell 3376 with Suzaku
DOI: 10.1051/0004-6361/201732496 Bibcode: 2018A&A...618A..74U

Urdampilleta, I.; Kaastra, J. S.; Mernier, F. +5 more

We present an X-ray spectral analysis of the nearby double radio relic merging cluster Abell 3376 (z = 0.046), observed with the Suzaku XIS instrument. These deep (∼360 ks) observations cover the entire double relic region in the outskirts of the cluster. These diffuse radio structures are amongst the largest and arc-shaped relics observed in comb…

2018 Astronomy and Astrophysics
Suzaku XMM-Newton 39
KiDS-SQuaD: The KiDS Strongly lensed Quasar Detection project
DOI: 10.1093/mnras/sty1923 Bibcode: 2018MNRAS.480.1163S

Koopmans, L. V. E.; Capaccioli, M.; Napolitano, N. R. +11 more

New methods have recently been developed to search for strong gravitational lenses, in particular lensed quasars, in wide-field imaging surveys. Here, we compare the performance of three different, morphology- and photometry-based methods to find lens candidates within the Kilo-Degree Survey (KiDS) DR3 footprint (440 deg2). The three me…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 39
Probing the Puzzle of Behind-the-limb γ-Ray Flares: Data-driven Simulations of Magnetic Connectivity and CME-driven Shock Evolution
DOI: 10.3847/1538-4357/aae1fd Bibcode: 2018ApJ...867..122J

Liu, Wei; Li, Gang; Jin, Meng +8 more

Recent detections of high-energy γ-rays from behind-the-limb (BTL) solar flares by the Fermi Gamma-ray Space Telescope pose a puzzle and challenge on the particle acceleration and transport mechanisms. In such events, the γ-ray emission region is located away from the BTL flare site by up to tens of degrees in heliographic longitude. It is thus hy…

2018 The Astrophysical Journal
SOHO 39
First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
DOI: 10.3847/1538-4357/aab3ca Bibcode: 2018ApJ...857...10A

Ward-Thompson, Derek; Fissel, Laura M.; Nakamura, Fumitaka +27 more

Polarized emission from aligned dust is a crucial tool for studies of magnetism in the ISM, but a troublesome contaminant for studies of cosmic microwave background polarization. In each case, an understanding of the significance of the polarization signal requires well-calibrated physical models of dust grains. Despite decades of progress in theo…

2018 The Astrophysical Journal
Planck 39
Interpretation of the Phase Functions Measured by the OSIRIS Instrument for Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/2041-8213/aaee10 Bibcode: 2018ApJ...868L..16M

Muinonen, Karri; Agarwal, Jessica; Penttilä, Antti +2 more

We show that the scattering phase functions of the coma and the nucleus of the comet 67P/Churyumov-Gerasimenko measured by the Rosetta/Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS) instrument can be reproduced by a particle model involving clustered, densely packed submicrometer-sized grains composed of organic material and l…

2018 The Astrophysical Journal
Rosetta 39
Dependence of Coronal Mass Ejection Properties on Their Solar Source Active Region Characteristics and Associated Flare Reconnection Flux
DOI: 10.3847/1538-4357/aada10 Bibcode: 2018ApJ...865....4P

Gopalswamy, Nat; Nandy, Dibyendu; Srivastava, Nandita +2 more

The near-Sun kinematics of coronal mass ejections (CMEs) determine the severity and arrival time of associated geomagnetic storms. We investigate the relationship between the deprojected speed and kinetic energy of CMEs and magnetic measures of their solar sources, reconnection flux of associated eruptive events, and intrinsic flux-rope characteri…

2018 The Astrophysical Journal
SOHO 39
The Morphological Evolution, AGN Fractions, Dust Content, Environments, and Downsizing of Massive Green Valley Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
DOI: 10.3847/1538-4357/aaad0b Bibcode: 2018ApJ...855...10G

Fang, Guanwen; Gu, Yizhou; Yuan, Qirong +2 more

To explore the evolutionary connection among red, green, and blue galaxy populations, based on a sample of massive ({M}* > {10}10 {M}) galaxies at 0.5 < z < 2.5 in five 3D-HST/CANDELS fields, we investigate the dust content, morphologies, structures, active galactic nucleus (AGN) fractions, and environme…

2018 The Astrophysical Journal
eHST 39