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Physical conditions in the gas phases of the giant H II region LMC-N 11. II. Origin of [C II] and fraction of CO-dark gas
DOI: 10.1051/0004-6361/201936303 Bibcode: 2019A&A...632A.106L

Lebouteiller, V.; Madden, S. C.; Galliano, F. +11 more

Context. The ambiguous origin of the [C II] 158µm line in the interstellar medium complicates its use for diagnostics concerning the star-formation rate and physical conditions in photodissociation regions.
Aims: We investigate the origin of [C II] in order to measure the total molecular gas content, the fraction of CO-dark H2

2019 Astronomy and Astrophysics
Herschel 14
The Eclipsing δ Scuti Star EPIC 245932119
DOI: 10.3847/1538-3881/aaf0fb Bibcode: 2019AJ....157...17L

Kristiansen, Martti H.; Hong, Kyeongsoo; Lee, Jae Woo

We present the physical properties of EPIC 245932119 (K p = +9.82) exhibiting both eclipses and pulsations from the K2 photometry. The binary modeling indicates that the eclipsing system is in detached or semi-detached configurations with a mass ratio of 0.283 or 0.245, respectively, and that its light-curve parameters are almost unaffe…

2019 The Astronomical Journal
Gaia 14
Sea level changes and vertical land motion from altimetry and tide gauges in the Southern Levantine Basin
DOI: 10.1016/j.jog.2019.05.007 Bibcode: 2019JGeo..128....1M

Mohamed, Bayoumy; Mohamed, Abdallah; Alam El-Din, Khaled +2 more

We have investigated the sea level rise (SLR) in the Southern Levantine region of the Mediterranean Sea during the period 1993-2015 using satellite altimetry and tide gauge data. Satellite altimetry indicated a positive SLR with a mean of 3.51 ± 0.62 mm/year, which is slightly higher than the global averaged mean SLR that was reported about 3.19 ±…

2019 Journal of Geodynamics
Rosetta 14
The HD 181433 Planetary System: Dynamics and a New Orbital Solution
DOI: 10.3847/1538-3881/ab2e78 Bibcode: 2019AJ....158..100H

Kane, Stephen R.; Wittenmyer, Robert A.; Horner, Jonathan +7 more

We present a detailed analysis of the orbital stability of the HD 181433 planetary system, finding it to exhibit strong dynamical instability across a wide range of orbital eccentricities, semimajor axes, and mutual inclinations. We also analyze the behavior of an alternative system architecture, proposed by Campanella, and find that it offers gre…

2019 The Astronomical Journal
Gaia 14
A systematic study of soft X-ray pulse profiles of magnetars in quiescence
DOI: 10.1093/mnras/stz513 Bibcode: 2019MNRAS.485.4274H

Ho, Wynn C. G.; Hu, Chin-Ping; Ng, C. -Y.

Magnetars are neutron stars with extremely high surface magnetic fields. They show diverse X-ray pulse profiles in the quiescent state. We perform a systematic Fourier analysis of their soft X-ray pulse profiles. We find that most magnetars have a single-peaked profile and hence have low amplitudes of the second Fourier harmonics (A2). …

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 14
Deep ugrizY imaging and DEEP2/3 spectroscopy: a photometric redshift testbed for LSST and public release of data from the DEEP3 Galaxy Redshift Survey
DOI: 10.1093/mnras/stz1866 Bibcode: 2019MNRAS.488.4565Z

Trump, Jonathan R.; Conselice, Christopher J.; Nandra, Kirpal +19 more

We present catalogues of calibrated photometry and spectroscopic redshifts in the Extended Groth Strip, intended for studies of photometric redshifts (photo-z's). The data includes ugriz photometry from Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) and Y-band photometry from the Subaru Suprime camera, as well as spectroscopic redshifts fro…

2019 Monthly Notices of the Royal Astronomical Society
eHST 14
Calibrating Star Formation Rate Prescriptions at Different Scales (10 pc-1 kpc) in M31
DOI: 10.3847/1538-4357/ab03ce Bibcode: 2019ApJ...873....3T

Schinnerer, Eva; Blanc, Guillermo A.; Kreckel, Kathryn +9 more

We calibrate commonly used star formation rate (SFR) prescriptions using observations in five kiloparsec-sized fields in the nearby galaxy Andromeda (M31) at 10 pc spatial resolution. Our observations at different scales enable us to resolve the star-forming regions and to distinguish them from non-star-forming components. We use extinction-correc…

2019 The Astrophysical Journal
Herschel 14
The MASSIVE Survey XIII. Spatially Resolved Stellar Kinematics in the Central 1 kpc of 20 Massive Elliptical Galaxies with the GMOS-North Integral Field Spectrograph
DOI: 10.3847/1538-4357/ab1f04 Bibcode: 2019ApJ...878...57E

Ma, Chung-Pei; Greene, Jenny E.; Blakeslee, John P. +5 more

We use observations from the GEMINI-N/GMOS integral field spectrograph (IFS) to obtain spatially resolved stellar kinematics of the central ∼1 kpc of 20 early-type galaxies (ETGs) with stellar masses greater than 1011.7 M in the MASSIVE survey. Together with observations from the wide-field Mitchell IFS at McDonald Observat…

2019 The Astrophysical Journal
eHST 14
Revealing dust-obscured star formation in CLJ1449+0856, a cluster at z = 2
DOI: 10.1093/mnras/stz1090 Bibcode: 2019MNRAS.486.4304S

Papageorgiou, A.; Smith, M. W. L.; Eales, S. A. +2 more

We present SCUBA-2 450 and 850 µm data of the mature redshift 2 cluster CLJ1449. We combine this with archival Herschel data to explore the star-forming properties of CLJ1449. Using high-resolution Atacama Large Millimetre Array and Jansky Very Large Array data we identify potentially confused galaxies, and use the Bayesian inference tool XI…

2019 Monthly Notices of the Royal Astronomical Society
Herschel 14
Discovery of a Lyα-emitting Dark Cloud within the z ∼ 2.8 SMM J02399-0136 System
DOI: 10.3847/1538-4357/ab0e6f Bibcode: 2019ApJ...875..130L

Ivison, R. J.; Prochaska, J. Xavier; Cai, Zheng +9 more

We present Keck/Keck Cosmic Web Imager (KCWI) integral field spectrograph observations of the complex system surrounding SMM J02399-0136 (a lensed z = 2.8 sub-mm galaxy), including an associated Lyα nebula, a dust-obscured, broad-absorption-line quasar, and neighboring galaxies. At a 3σ surface brightness contour of 1.6 × 10-17 erg s

2019 The Astrophysical Journal
eHST 14