Search Publications

First Assessment of the Binary Lens OGLE-2015-BLG-0232
DOI: 10.3847/1538-4357/aaedb9 Bibcode: 2019ApJ...870...11B

Bennett, D. P.; Soszyński, I.; Udalski, A. +54 more

We present an analysis of the microlensing event OGLE-2015-BLG-0232. This event is challenging to characterize for two reasons. First, the light curve is not well sampled during the caustic crossing due to the proximity of the full Moon impacting the photometry quality. Moreover, the source brightness is difficult to estimate because this event is…

2019 The Astrophysical Journal
Gaia 10
Electron Densities and Nitrogen Abundances in Ionized Gas Derived Using [N II] Fine-structure and Hydrogen Recombination Lines
DOI: 10.3847/1538-4357/ab46c2 Bibcode: 2019ApJ...886....1P

Lazio, T. Joseph W.; Horiuchi, Shinji; Goldsmith, Paul F. +7 more

We present a method for deriving the electron density of ionized gas using the ratio of the intensity of the [N II] 205 µm line to that of hydrogen radio recombination lines (RRLs). We use this method to derive electron densities of 21 velocity components in 11 lines of sight through the Galaxy, including the Galactic center. We observed, at…

2019 The Astrophysical Journal
Herschel 10
Member Stars of the GD-1 Tidal Stream from the SDSS, LAMOST, and Gaia Surveys
DOI: 10.3847/1538-4357/ab158a Bibcode: 2019ApJ...877...13H

Huang, Y.; Chen, B. -Q.; Wang, C. +5 more

With the photometric data from the SDSS survey, the spectroscopic data from the SDSS/SEGUE and the LAMOST surveys, and the astrometric data from the Gaia DR2, we have identified 67 highly probable member stars of the GD-1 cold stellar stream spread along almost its entire length (i.e., from 126° to 203° in R.A.). With the accurate spectroscopic (i…

2019 The Astrophysical Journal
Gaia 10
Carbon-deficient Red Giants
DOI: 10.3847/1538-4357/ab4e13 Bibcode: 2019ApJ...887...12B

Bond, Howard E.

Carbon-deficient red giants (CDRGs) are a rare class of peculiar red giants, also called “weak G-band” or “weak CH” stars. Their atmospheric compositions show depleted carbon, a low {}12{{C}}{/}13{{C}} isotopic ratio, and an overabundance of nitrogen, indicating that the material at the surface has undergone CN-cycle hydrogen…

2019 The Astrophysical Journal
Gaia 10
On Geometrical Invariants of the Magnetic Field Gradient Tensor in Turbulent Space Plasmas: Scale Variability in the Inertial Range
DOI: 10.3847/1538-4357/ab1e47 Bibcode: 2019ApJ...878..124Q

Marcucci, Maria Federica; Consolini, Giuseppe; Materassi, Massimo +1 more

In a recent paper, Consolini et al. investigated the statistics of geometrical invariants of the coarse-grained gradient tensor of plasma velocity for a case study of space plasma turbulence. They showed how, at spatial scales near the proton inertial length, there is evidence for the occurrence of dissipation structures along the Vieillefosse’s t…

2019 The Astrophysical Journal
Cluster 10
Asymmetric Distribution of Weak Photospheric Magnetic Field Values
DOI: 10.3847/1538-4357/ab0749 Bibcode: 2019ApJ...874..116G

Mursula, Kalevi; Virtanen, Ilpo; Getachew, Tibebu

We use the synoptic maps of the photospheric magnetic field observed at Wilcox Solar Observatory, Mount Wilson Observatory, Kitt Peak, SOHO/MDI, SOLIS/VSM, and SDO/HMI to study the distribution of weak photospheric magnetic field values in 1974-2018. We fit the histogram distribution of weak field values for each synoptic map of the six data sets …

2019 The Astrophysical Journal
SOHO 10
Measuring the Obscuring Column of a Disk Megamaser AGN in a Nearby Merger
DOI: 10.3847/1538-4357/ab3214 Bibcode: 2019ApJ...882...83M

Comastri, A.; Brusa, M.; Civano, F. +5 more

Active galactic nuclei (AGNs) hosting disk water megamasers are well known to be obscured by large amounts of gas, likely due to the presence along the line of sight of an almost edge-on disky structure orbiting the supermassive black hole. Correcting for the high obscuration is crucial to infer parameters intrinsic to the source, like its luminos…

2019 The Astrophysical Journal
eHST 10
Discovery of a Damped Lyα System in a Low-z Galaxy Group: Possible Evidence for Gas Inflow and Nuclear Star Formation
DOI: 10.3847/1538-4357/aaf566 Bibcode: 2019ApJ...871..239B

Heckman, Timothy M.; Tumlinson, Jason; Momjian, Emmanuel +3 more

We present a low-redshift (z = 0.029) damped Lyα (DLA) system in the spectrum of a background quasi-stellar object (QSO). The DLA is associated with an interacting galaxy pair within a galaxy group. We detected weak Lyα emission centered at the absorption trough of the DLA. The emission was likely tracing the neutral H I reservoir around the galax…

2019 The Astrophysical Journal
eHST 10
Catalog of High Protostellar Surface Density Regions in Nearby Embedded Clusters
DOI: 10.3847/1538-4357/aaf652 Bibcode: 2019ApJ...871..163L

Li, Juan; Myers, Philip C.; Kirk, Helen +3 more

We analyze high-quality stellar catalogs for 24 young and nearby (within 1 kpc) embedded clusters and present a catalog of 32 groups which have a high concentration of protostars. The median effective radius of these groups is 0.17 pc. The median protostellar and pre-main-sequence star surface densities are 46 M pc-2 and 11…

2019 The Astrophysical Journal
Herschel 10
T CrB: Radio Observations during the 2016-2017 “Super-active” State
DOI: 10.3847/1538-4357/ab3c62 Bibcode: 2019ApJ...884....8L

Chomiuk, Laura; Sokoloski, Jennifer L.; Mukai, Koji +6 more

We obtained radio observations of the symbiotic binary and known recurrent nova T Coronae Borealis following a period of increased activity in the optical and X-ray bands. A comparison of our observations with those made prior to 2015 indicates that the system is in a state of higher emission in the radio as well. The spectral energy distributions…

2019 The Astrophysical Journal
Gaia 10