Search Publications

Two Small Transiting Planets and a Possible Third Body Orbiting HD 106315
DOI: 10.3847/1538-3881/aa6e01 Bibcode: 2017AJ....153..255C

de Pater, Imke; Knutson, Heather A.; Schlieder, Joshua E. +21 more

The masses, atmospheric makeups, spin-orbit alignments, and system architectures of extrasolar planets can be best studied when the planets orbit bright stars. We report the discovery of three bodies orbiting HD 106315, a bright (V = 8.97 mag) F5 dwarf targeted by our K2 survey for transiting exoplanets. Two small transiting planets are found to h…

2017 The Astronomical Journal
Gaia 37
Type 2 AGN Host Galaxies in the Chandra-COSMOS Legacy Survey: No Evidence of AGN-driven Quenching
DOI: 10.3847/1538-4357/aa725c Bibcode: 2017ApJ...841..102S

Schawinski, Kevin; Elvis, Martin; Lusso, Elisabeta +16 more

We investigate the star formation properties of a large sample of ∼2300 X-ray-selected Type 2 Active Galactic Nuclei (AGNs) host galaxies out to z∼ 3 in the Chandra COSMOS Legacy Survey in order to understand the connection between the star formation and nuclear activity. Making use of the existing multi-wavelength photometric data available in th…

2017 The Astrophysical Journal
Herschel 37
ALMA imaging of C2H emission in the disk of NGC 1068
DOI: 10.1051/0004-6361/201731862 Bibcode: 2017A&A...608A..56G

Tacconi, L. J.; Hunt, L. K.; Krips, M. +16 more


Aims: We study the feedback of star formation and nuclear activity on the chemistry of molecular gas in NGC 1068, a nearby (D = 14 Mpc) Seyfert 2 barred galaxy, by analyzing whether the abundances of key molecular species such as ethynyl (C2H), which is a classical tracer of photon dominated regions (PDR), change in the different e…

2017 Astronomy and Astrophysics
eHST 37
First Scattered-light Images of the Gas-rich Debris Disk around 49 Ceti
DOI: 10.3847/2041-8213/834/2/L12 Bibcode: 2017ApJ...834L..12C

Debes, John H.; Roberge, Aki; Schneider, Glenn +31 more

We present the first scattered-light images of the debris disk around 49 Ceti, a ∼40 Myr A1 main-sequence star at 59 pc, famous for hosting two massive dust belts as well as large quantities of atomic and molecular gas. The outer disk is revealed in reprocessed archival Hubble Space Telescope NICMOS-F110W images, as well as new coronagraphic H-ban…

2017 The Astrophysical Journal
eHST 37
Global Solar Magnetic Field Organization in the Outer Corona: Influence on the Solar Wind Speed and Mass Flux Over the Cycle
DOI: 10.3847/1538-4357/aa9218 Bibcode: 2017ApJ...850...45R

Réville, Victor; Brun, Allan Sacha

The dynamics of the solar wind depends intrinsically on the structure of the global solar magnetic field, which undergoes fundamental changes over the 11-year solar cycle. For instance, the wind terminal velocity is thought to be anti-correlated with the expansion factor, a measure of how the magnetic field varies with height in the solar corona, …

2017 The Astrophysical Journal
Ulysses 37
Modulation of Galactic Cosmic Rays in the Inner Heliosphere, Comparing with PAMELA Measurements
DOI: 10.3847/1538-4357/aa83ad Bibcode: 2017ApJ...846...56Q

Qin, G.; Shen, Z. -N.

We develop a numerical model to study the time-dependent modulation of galactic cosmic rays in the inner heliosphere. In the model, a time-delayed modified Parker heliospheric magnetic field (HMF) and a new diffusion coefficient model, NLGCE-F, from Qin & Zhang, are adopted. In addition, the latitudinal dependence of magnetic turbulence magnit…

2017 The Astrophysical Journal
Ulysses 37
The Properties of the Galactic Hot Gaseous Halo from X-Ray Emission
DOI: 10.3847/1538-4357/aa92c6 Bibcode: 2017ApJ...849..105L

Li, Yunyang; Bregman, Joel

The extended hot X-ray emitting gaseous halo of the Milky Way has an optical depth ∼1 for the dominant emission lines of O vii and O viii, which are used to infer the halo properties. To improve on halo gas properties, we treat optical depth effects with a Monte Carlo radiative transfer model, which leads to slightly steeper density profiles (β ≈ …

2017 The Astrophysical Journal
XMM-Newton 37
Restarting activity in the nucleus of PBC J2333.9-2343. An extreme case of jet realignment
DOI: 10.1051/0004-6361/201730530 Bibcode: 2017A&A...603A.131H

Ghisellini, G.; Masetti, N.; Giroletti, M. +8 more

Context. The giant radio galaxy PBC J2333.9-2343 shows different characteristics at different wavebands that are difficult to explain within the actual generic schemes of unification of active galactic nuclei (AGN). It is therefore a good candidate host for different phases of nuclear activity.
Aims: We aim at disentangling the nature of this…

2017 Astronomy and Astrophysics
XMM-Newton 37
Surge-like Oscillations above Sunspot Light Bridges Driven by Magnetoacoustic Shocks
DOI: 10.3847/1538-4357/aa63e8 Bibcode: 2017ApJ...838....2Z

He, Jiansen; Tian, Hui; Zhang, Jingwen +1 more

High-resolution observations of the solar chromosphere and transition region often reveal surge-like oscillatory activities above sunspot light bridges (LBs). These oscillations are often interpreted as intermittent plasma jets produced by quasi-periodic magnetic reconnection. We have analyzed the oscillations above an LB in a sunspot using data t…

2017 The Astrophysical Journal
IRIS 37
Constraints on cometary surface evolution derived from a statistical analysis of 67P's topography
DOI: 10.1093/mnras/stx1691 Bibcode: 2017MNRAS.469S.329V

Jorda, L.; Lamy, P. L.; Lara, L. M. +51 more

We present a statistical analysis of the distribution of large-scale topographic features on comet 67P/Churyumov-Gerasimenko. We observe that the cumulative cliff height distribution across the surface follows a power law with a slope equal to -1.69 ± 0.02. When this distribution is studied independently for each region, we find a good correlation…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 37