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Resolved Neutral Carbon Emission in Nearby Galaxies: [C I] Lines as Total Molecular Gas Tracers
DOI: 10.3847/1538-4357/ab29ed Bibcode: 2019ApJ...880..133J

Tan, Qinghua; Salak, Dragan; Gao, Yu +6 more

We present maps of atomic carbon [C I]({}3{{{P}}}1\to {{}3{{P}}}0) and [C I]({}3{{{P}}}2\to {{}3{{P}}}1) emission (hereafter [C I] (1-0) and [C I] (2-1), respectively) at a linear resolution ∼1 kpc scale for a sample of one H II, six LINER, three Seyfert, and f…

2019 The Astrophysical Journal
Herschel 43
Transition Probabilities of Sc I and Sc II and Scandium Abundances in the Sun, Arcturus, and HD 84937
DOI: 10.3847/1538-4365/ab08ef Bibcode: 2019ApJS..241...21L

Sneden, C.; Wood, M. P.; Lawler, J. E. +3 more

New branching fraction (BF) measurements for lines of Sc I and Sc II from 24 Fourier transform spectra calibrated using standard lamps and the Ar branching ratio method are reported. The BFs for 259 lines are converted to absolute atomic transition probabilities using published radiative lifetimes from laser-induced fluorescence measurements. Deta…

2019 The Astrophysical Journal Supplement Series
eHST 43
Crossing the Line: Active Galactic Nuclei in the Star-forming Region of the BPT Diagram
DOI: 10.3847/1538-4357/ab1094 Bibcode: 2019ApJ...876...12A

Salim, Samir; Agostino, Christopher J.

In this work, we investigate the reliability of the BPT diagram for excluding galaxies that host an active galactic nucleus (AGN). We determine the prevalence of X-ray AGNs in the star-forming region of the BPT diagram and discuss the reasons behind this apparent misclassification, focusing primarily on relatively massive ({log}({M}* )≳…

2019 The Astrophysical Journal
XMM-Newton 43
Dramatic spectral transition of X-ray pulsar GX 304-1 in low luminous state
DOI: 10.1093/mnrasl/sly236 Bibcode: 2019MNRAS.483L.144T

Doroshenko, Victor; Tsygankov, Sergey S.; Mushtukov, Alexander A. +5 more

We report on the discovery of a dramatic change in the energy spectrum of the X-ray pulsar GX 304-1 appearing at low luminosity. Particularly, we found that the cut-off power-law spectrum typical for accreting pulsars, including GX 304-1 at higher luminosities of LX ∼ 1036-1037 erg s-1, transformed at lo…

2019 Monthly Notices of the Royal Astronomical Society
INTEGRAL 43
Type Ibn Supernovae May not all Come from Massive Stars
DOI: 10.3847/2041-8213/aafc61 Bibcode: 2019ApJ...871L...9H

Zabludoff, Ann I.; French, K. Decker; Berger, Edo +5 more

Because core-collapse supernovae are the explosions of massive stars, which have relatively short lifetimes, they occur almost exclusively in galaxies with active star formation. On the other hand, the Type Ibn supernova PS1-12sk exploded in an environment that is much more typical of thermonuclear (Type Ia) supernovae: on the outskirts of the bri…

2019 The Astrophysical Journal
eHST 43
More than two hundred and fifty thousand spectroscopic binary or variable star candidates discovered by LAMOST
DOI: 10.1088/1674-4527/19/5/64 Bibcode: 2019RAA....19...64Q

Li, Lin-Jia; Qian, Sheng-Bang; Zhu, Li-Ying +7 more

About 786.4 thousand stars were observed by LAMOST twice or more during the first stage of its spectroscopic survey. The radial velocity differences for about 256 thousand targets are larger than 10 km s-1 and they are possible spectroscopic binary or variable candidates (SBVCs). It is shown that most SBVCs are slightly metal poorer tha…

2019 Research in Astronomy and Astrophysics
Gaia 43
Contrast sensitivities in the Gaia Data Release 2
DOI: 10.1051/0004-6361/201834321 Bibcode: 2019A&A...621A..86B

Cataldi, Gianni; Brandeker, Alexis

The source detection sensitivity of Gaia is reduced near sources. To characterise this contrast sensitivity is important for understanding the completeness of the Gaia data products, in particular when evaluating source confusion in lower resolution surveys such as photometric monitoring for transits. Here, we statistically evaluate the catalogue …

2019 Astronomy and Astrophysics
Gaia 43
Interstellar Neutral Gas Species and Their Pickup Ions inside the Heliospheric Termination Shock. Ionization Rates for H, O, Ne, and He
DOI: 10.3847/1538-4357/aafdaf Bibcode: 2019ApJ...872...57S

Tokumaru, Munetoshi; Bzowski, Maciej; Sokół, Justyna M.

Solar ionizing factors are responsible for modulation of interstellar neutral gas and its derivative populations inside the heliosphere. We provide an overview of the current state of knowledge about them for heliospheric particles inside the termination shock. We discuss charge exchange with solar wind particles, photoionization, and electron imp…

2019 The Astrophysical Journal
Ulysses 43
Torus model properties of an ultra-hard X-ray selected sample of Seyfert galaxies
DOI: 10.1093/mnras/stz1003 Bibcode: 2019MNRAS.486.4917G

Hernán-Caballero, A.; Carrera, F. J.; Acosta-Pulido, J. A. +15 more

We characterize for the first time the torus properties of an ultra-hard X-ray (14-195 keV) volume-limited (DL < 40 Mpc) sample of 24 Seyfert (Sy) galaxies (BCS40 sample). The sample was selected from the Swift/BAT nine-month catalogue. We use high angular resolution nuclear infrared (IR) photometry and N-band spectroscopy…

2019 Monthly Notices of the Royal Astronomical Society
eHST 43
Binospec Software System
DOI: 10.1088/1538-3873/ab1ceb Bibcode: 2019PASP..131g5005K

Chilingarian, Igor; Paegert, Martin; Fabricant, Daniel +6 more

Binospec is a high-throughput, 370 to 1000 nm, imaging spectrograph that addresses two adjacent 8‧ by 15‧ fields of view. Binospec was commissioned in late 2017 at the f/5 focus of the 6.5 m MMT and is now available to all MMT observers. Here we describe the Binospec software used for observation planning, instrument control, and data reduction. T…

2019 Publications of the Astronomical Society of the Pacific
Gaia 43