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HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625
DOI: 10.1051/0004-6361/201730957 Bibcode: 2017A&A...605A..92S

Rebolo, R.; Ribas, I.; Morales, J. C. +27 more

We report the discovery of a super-Earth orbiting at the inner edge of the habitable zone of the star GJ 625 based on the analysis of the radial-velocity (RV) time series from the HARPS-N spectrograph, consisting of 151 HARPS-N measurements taken over 3.5 yr. GJ 625 b is a planet with a minimum mass Msini of 2.82 ± 0.51 M with an orbit…

2017 Astronomy and Astrophysics
Gaia 31
A decade of warm hot intergalactic medium searches: Where do we stand and where do we go?
DOI: 10.1002/asna.201713343 Bibcode: 2017AN....338..281N

Elvis, M.; Nicastro, F.; Krongold, Y. +1 more

In this article, we first review the past decade of efforts in detecting the missing baryons in the warm hot intergalactic medium and summarize the current state of the art by updating the baryon census and physical state of the detected baryons in the local Universe. We then describe observational strategies that should enable a significant step …

2017 Astronomische Nachrichten
XMM-Newton 31
Onset of a Large Ejective Solar Eruption from a Typical Coronal-jet-base Field Configuration
DOI: 10.3847/1538-4357/aa7c1b Bibcode: 2017ApJ...845...26J

Moon, Yong-Jae; Joshi, Navin Chandra; Magara, Tetsuya +2 more

Utilizing multiwavelength observations and magnetic field data from the Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly (AIA), SDO/Helioseismic and Magnetic Imager (HMI), the Geostationary Operational Environmental Satellite (GOES), and RHESSI, we investigate a large-scale ejective solar eruption of 2014 December 18 from active regio…

2017 The Astrophysical Journal
SOHO 31
Spectral and timing properties of IGR J00291+5934 during its 2015 outburst
DOI: 10.1093/mnras/stw3332 Bibcode: 2017MNRAS.466.2910S

Sanna, A.; Egron, E.; Ferrigno, C. +8 more

We report on the spectral and timing properties of the accreting millisecond X-ray pulsar IGR J00291+5934 observed by XMM-Newton and NuSTAR during its 2015 outburst. The source is in a hard state dominated at high energies by a Comptonization of soft photons (∼0.9 keV) by an electron population with kTe ∼ 30 keV, and at lower energies b…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 31
NGC 1566: analysis of the nuclear region from optical and near-infrared Integral Field Unit spectroscopy
DOI: 10.1093/mnras/stx1458 Bibcode: 2017MNRAS.470.3850D

Steiner, J. E.; Menezes, R. B.; da Silva, Patrícia

We analysed the centre of NGC 1566, which hosts a well-studied active galactic nucleus (AGN), known for its variability. With the aid of techniques such as Principal Component Analysis Tomography, analysis of the emission-line spectra, channel maps, Penalized Pixel Fitting and spectral synthesis applied to the optical and near-infrared data cubes,…

2017 Monthly Notices of the Royal Astronomical Society
eHST 30
Lens Model and Time Delay Predictions for the Sextuply Lensed Quasar SDSS J2222+2745
DOI: 10.3847/1538-4357/835/1/5 Bibcode: 2017ApJ...835....5S

Rigby, Jane R.; Whitaker, Katherine E.; Sharon, Keren +7 more

SDSS J2222+2745 is a galaxy cluster at z = 0.49, strongly lensing a quasar at z = 2.805 into six widely separated images. In recent Hubble Space Telescope imaging of the field, we identify additional multiply lensed galaxies and confirm the sixth quasar image that was identified by Dahle et al. We used the Gemini-North telescope to measure a spect…

2017 The Astrophysical Journal
eHST 30
Orbits for 18 Visual Binaries and Two Double-line Spectroscopic Binaries Observed with HRCAM on the CTIO SOAR 4 m Telescope, Using a New Bayesian Orbit Code Based on Markov Chain Monte Carlo
DOI: 10.3847/1538-3881/aa8d6f Bibcode: 2017AJ....154..187M

Mendez, Rene A.; Claveria, Ruben M.; Orchard, Marcos E. +1 more

We present orbital elements and mass sums for 18 visual binary stars of spectral types B to K (five of which are new orbits) with periods ranging from 20 to more than 500 yr. For two double-line spectroscopic binaries with no previous orbits, the individual component masses, using combined astrometric and radial velocity data, have a formal uncert…

2017 The Astronomical Journal
Gaia 30
Two-Step Filament Eruption During 14 - 15 March 2015
DOI: 10.1007/s11207-017-1104-5 Bibcode: 2017SoPh..292...81C

Filippov, B.; Schmieder, B.; Chandra, R. +1 more

We present here an interesting two-step filament eruption during 14 - 15 March 2015. The filament was located in NOAA AR 12297 and associated with a halo Coronal Mass Ejection (CME). We use observations from the Atmospheric Imaging Assembly (AIA) and Heliospheric Magnetic Imager (HMI) instruments onboard the Solar Dynamics Observatory (SDO), and f…

2017 Solar Physics
SOHO 30
The Architecture of the GW Ori Young Triple-star System and Its Disk: Dynamical Masses, Mutual Inclinations, and Recurrent Eclipses
DOI: 10.3847/1538-4357/aa9be7 Bibcode: 2017ApJ...851..132C

Torres, Guillermo; Latham, David W.; Wilner, David J. +15 more

We present spatially and spectrally resolved Atacama Large Millimeter/submillimeter Array (ALMA) observations of gas and dust orbiting the pre-main-sequence hierarchical triple-star system GW Ori. A forward modeling of the 13CO and C18O J = 2-1 transitions permits a measurement of the total stellar mass in this system, 5.29+/…

2017 The Astrophysical Journal
Gaia 30
The Coldest Place in the Universe: Probing the Ultra-cold Outflow and Dusty Disk in the Boomerang Nebula
DOI: 10.3847/1538-4357/aa6d86 Bibcode: 2017ApJ...841..110S

Sahai, R.; Vlemmings, W. H. T.; Nyman, L. -Å.

Our Cycle 0 ALMA observations confirmed that the Boomerang Nebula is the coldest known object in the universe, with a massive high-speed outflow that has cooled significantly below the cosmic background temperature. Our new CO 1-0 data reveal heretofore unseen distant regions of this ultra-cold outflow, out to ≳120,000 au. We find that in the ultr…

2017 The Astrophysical Journal
eHST 30