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A Review on Substellar Objects below the Deuterium Burning Mass Limit: Planets, Brown Dwarfs or What?
DOI: 10.3390/geosciences8100362 Bibcode: 2018Geosc...8..362C

Caballero, José A.

"Free-floating, non-deuterium-burning, substellar objects" are isolated bodies of a few Jupiter masses found in very young open clusters and associations, nearby young moving groups and in the immediate vicinity of the Sun. They are neither brown dwarfs nor planets. I look over their nomenclature, history of discovery, sites of detection, formatio…

2018 Geosciences
Gaia 28
Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246-0526
DOI: 10.3847/1538-4357/aae698 Bibcode: 2018ApJ...868...15T

Tsai, Chao-Wei; Wright, Edward L.; Jun, Hyunsung D. +8 more

We use optical and near-infrared spectroscopy to observe rest-UV emission lines and estimate the black hole mass of WISEA J224607.56-052634.9 (W2246-0526) at z = 4.601, the most luminous hot, dust-obscured galaxy yet discovered by WISE. From the broad component of the Mg II 2799 Å emission line, we measure a black hole mass of log(M BH/…

2018 The Astrophysical Journal
eHST 28
The APOGEE-2 Survey of the Orion Star-forming Complex. I. Target Selection and Validation with Early Observations
DOI: 10.3847/1538-4365/aabada Bibcode: 2018ApJS..236...27C

Da Rio, Nicola; Pan, Kaike; Majewski, Steven R. +26 more

The Orion Star-forming Complex (OSFC) is a central target for the APOGEE-2 Young Cluster Survey. Existing membership catalogs span limited portions of the OSFC, reflecting the difficulty of selecting targets homogeneously across this extended, highly structured region. We have used data from wide-field photometric surveys to produce a less biased …

2018 The Astrophysical Journal Supplement Series
XMM-Newton 28
A radiation belt of energetic protons located between Saturn and its rings
DOI: 10.1126/science.aat1962 Bibcode: 2018Sci...362.1962R

Livi, S.; Krupp, N.; Jones, G. H. +21 more

Saturn has a sufficiently strong dipole magnetic field to trap high-energy charged particles and form radiation belts, which have been observed outside its rings. Whether stable radiation belts exist near the planet and inward of the rings was previously unknown. The Cassini spacecraft's Magnetosphere Imaging Instrument obtained measurements of a …

2018 Science
Cassini 28
KiDS-i-800: comparing weak gravitational lensing measurements from same-sky surveys
DOI: 10.1093/mnras/sty859 Bibcode: 2018MNRAS.477.4285A

Heymans, C.; Wolf, C.; Lidman, C. +21 more

We present a weak gravitational lensing analysis of 815 deg2 of i-band imaging from the Kilo-Degree Survey (KiDS-i-800). In contrast to the deep r-band observations, which take priority during excellent seeing conditions and form the primary KiDS data set (KiDS-r-450), the complementary yet shallower KiDS-i-800 spans a wide range of obs…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 28
On the production of He, C, and N by low- and intermediate-mass stars: a comparison of observed and model-predicted planetary nebula abundances
DOI: 10.1093/mnras/stx2286 Bibcode: 2018MNRAS.473..241H

Balick, B.; Henry, R. B. C.; Stephenson, B. G. +2 more

The primary goal of this paper is to make a direct comparison between the measured and model-predicted abundances of He, C, and N in a sample of 35 well-observed Galactic planetary nebulae (PNe). All observations, data reductions, and abundance determinations were performed in house to ensure maximum homogeneity. Progenitor star masses (M ≤ 4 M

2018 Monthly Notices of the Royal Astronomical Society
IUE eHST 28
An ALMA Survey of Faint Disks in the Chamaeleon I Star-forming Region: Why Are Some Class II Disks so Faint?
DOI: 10.3847/1538-4357/aacce9 Bibcode: 2018ApJ...863...61L

Pascucci, Ilaria; Herczeg, Gregory J.; Henning, Thomas +6 more

ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate either different evolutionary paths of disks or different initial conditions within a single cluster. We present ALMA Cycle 3 follow-up observations for 14 Class II disks t…

2018 The Astrophysical Journal
Gaia 27
Investigating the volcanic versus aqueous origin of the surficial deposits in Eastern Elysium Planitia, Mars
DOI: 10.1016/j.icarus.2018.03.009 Bibcode: 2018Icar..309..389V

Voigt, Joana R. C.; Hamilton, Christopher W.

The Elysium Volcanic Province consists of numerous overlapping flow units and may include the youngest lava flows on Mars. However, it is possible that these volcanic units have been modified or overprinted by aqueous processes. Understanding the timing of the igneous and aqueous events in this region is therefore essential for constraining the ge…

2018 Icarus
MEx 27
Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system
DOI: 10.1093/mnras/sty1193 Bibcode: 2018MNRAS.478.4720G

Smalley, Barry; Gibson, Neale P.; Wheatley, Peter J. +36 more

We present the discovery of NGTS-3Ab, a hot Jupiter found transiting the primary star of an unresolved binary system. We develop a joint analysis of multicolour photometry, centroids, radial velocity (RV) cross-correlation function (CCF) profiles, and their bisector inverse slopes (BIS) to disentangle this three-body system. Data from the Next Gen…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 27
Star formation in the outskirts of DDO 154: a top-light IMF in a nearly dormant disc
DOI: 10.1093/mnras/sty1006 Bibcode: 2018MNRAS.477.5554W

Meurer, Gerhardt R.; Lagos, Claudia D. P.; Kroupa, Pavel +3 more

We present optical photometry of Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS)/Wide Field Camera (WFC) data of the resolved stellar populations in the outer disc of the dwarf irregular galaxy DDO 154. The photometry reveals that young main sequence (MS) stars are almost absent from the outermost H I disc. Instead, most are cluster…

2018 Monthly Notices of the Royal Astronomical Society
eHST 27