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Distances to the Globular Clusters 47 Tucanae and NGC 362 Using Gaia DR2 Parallaxes
DOI: 10.3847/1538-4357/aae089 Bibcode: 2018ApJ...867..132C

Caiazzo, Ilaria; Chen, Seery; Heyl, Jeremy +1 more

Using parallaxes from Gaia Data Release 2 (Gaia DR2), we estimate the distance to the globular clusters 47 Tuc and NGC 362, taking advantage of the background stars in the Small Magellanic Cloud and quasars to account for various parallax systematics. We found the parallax to be dependent on the Gaia DR2 G-band apparent magnitude for stars with 13…

2018 The Astrophysical Journal
Gaia 54
A Review of Alfvénic Turbulence in High-Speed Solar Wind Streams: Hints From Cometary Plasma Turbulence
DOI: 10.1002/2017JA024203 Bibcode: 2018JGRA..123.2458T

Hellinger, Petr; Tsurutani, Bruce T.; Glassmeier, Karl-Heinz +3 more

Solar wind turbulence within high-speed streams is reviewed from the point of view of embedded single nonlinear Alfvén wave cycles, discontinuities, magnetic decreases (MDs), and shocks. For comparison and guidance, cometary plasma turbulence is also briefly reviewed. It is demonstrated that cometary nonlinear magnetosonic waves phase-steepen, wit…

2018 Journal of Geophysical Research (Space Physics)
Cluster 54
The Rotation and Interior Structure Experiment on the InSight Mission to Mars
DOI: 10.1007/s11214-018-0530-5 Bibcode: 2018SSRv..214..100F

Golombek, Matthew P.; Asmar, Sami W.; Yseboodt, Marie +5 more

The Rotation and Interior Structure Experiment (RISE) on-board the InSight mission will use the lander's X-band (8 GHz) radio system in combination with tracking stations of the NASA Deep Space Network (DSN) to determine the rotation of Mars. RISE will measure the nutation of the Martian spin axis, detecting for the first time the effect of the li…

2018 Space Science Reviews
MEx 54
The structure of post-starburst galaxies at 0.5 < z < 2: evidence for two distinct quenching routes at different epochs
DOI: 10.1093/mnras/sty1794 Bibcode: 2018MNRAS.480..381M

Simpson, Chris; Wild, Vivienne; Almaini, Omar +5 more

We present an analysis of the structure of post-starburst (PSB) galaxies in the redshift range 0.5 < z < 2, using a photometrically selected sample identified in the Ultra Deep Survey field. We examine the structure of ∼80 of these transient galaxies using radial light µ(r) profiles obtained from CANDELS Hubble Space Telescope near-inf…

2018 Monthly Notices of the Royal Astronomical Society
eHST 54
Successive Flux Rope Eruptions from δ-sunspots Region of NOAA 12673 and Associated X-class Eruptive Flares on 2017 September 6
DOI: 10.3847/1538-4357/aaed26 Bibcode: 2018ApJ...869...69M

Joshi, Bhuwan; Veronig, Astrid M.; Mitra, Prabir K. +2 more

In this article, we present a multiwavelength analysis of two X-class solar eruptive flares of classes X2.2 and X9.3 that occurred in the sigmoidal active region NOAA 12673 on 2017 September 6, by combining observations of Atmospheric Imaging Assembly and Helioseismic Magnetic Imager instruments on board the Solar Dynamics Observatory. On the day …

2018 The Astrophysical Journal
SOHO 54
LOFAR-Boötes: properties of high- and low-excitation radio galaxies at 0.5 < z < 2.0
DOI: 10.1093/mnras/sty026 Bibcode: 2018MNRAS.475.3429W

Prandoni, I.; White, G. J.; Tasse, C. +13 more

This paper presents a study of the redshift evolution of radio-loud active galactic nuclei (AGN) as a function of the properties of their galaxy hosts in the Boötes field. To achieve this we match low-frequency radio sources from deep 150-MHz LOFAR (LOw Frequency ARray) observations to an I-band-selected catalogue of galaxies, for which we have de…

2018 Monthly Notices of the Royal Astronomical Society
Herschel 54
Hydrogen and Sodium Absorption in the Optical Transmission Spectrum of WASP-12b
DOI: 10.3847/1538-3881/aadca7 Bibcode: 2018AJ....156..154J

Cochran, William D.; Endl, Michael; Redfield, Seth +2 more

We have obtained >10 hr of medium-resolution (R ∼ 15,000) spectroscopic exposures on the transiting exoplanet host star WASP-12, including ∼2 hr while its planet, WASP-12b, is in transit, with the Hobby-Eberly Telescope. The out-of-transit and in-transit spectra are coadded into master out-of-transit and in-transit spectra, from which we create…

2018 The Astronomical Journal
Gaia 54
Direct imaging of an ultracool substellar companion to the exoplanet host star HD 4113 A
DOI: 10.1051/0004-6361/201630136 Bibcode: 2018A&A...614A..16C

Ségransan, D.; Delisle, J. -B.; Udry, S. +7 more

Using high-contrast imaging with the SPHERE instrument at the Very Large Telescope (VLT), we report the first images of a cold brown dwarf companion to the exoplanet host star HD 4113A. The brown dwarf HD 4113C is part of a complex dynamical system consisting of a giant planet, a stellar host, and a known wide M-dwarf companion. Its separation of …

2018 Astronomy and Astrophysics
Gaia 54
Does the X-ray outflow quasar PDS 456 have a UV outflow at 0.3c?
DOI: 10.1093/mnras/sty043 Bibcode: 2018MNRAS.476..943H

Hamann, Fred; Nardini, Emanuele; Reeves, James +1 more

The quasar PDS 456 (at redshift ∼0.184) has a prototype ultra-fast outflow (UFO) measured in X-rays. This outflow is highly ionized with relativistic speeds, large total column densities log NH(cm-2) > 23, and large kinetic energies that could be important for feedback to the host galaxy. A UV spectrum of PDS 456 obtained …

2018 Monthly Notices of the Royal Astronomical Society
eHST 54
The Carnegie-Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch
DOI: 10.3847/1538-4357/aa9d92 Bibcode: 2018ApJ...852...60J

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +8 more

The Carnegie-Chicago Hubble Program (CCHP) seeks to anchor the distance scale of Type Ia supernovae via the Tip of the Red Giant Branch (TRGB) method. Based on deep Hubble Space Telescope ACS/WFC imaging, we present an analysis of the TRGB for the metal-poor halo of NGC 1365, a giant spiral galaxy in the Fornax cluster that was host to the Type Ia…

2018 The Astrophysical Journal
eHST 54