Search Publications

The COS Absorption Survey of Baryon Harbors: The Galaxy Database and Cross-correlation Analysis of O VI Systems
DOI: 10.3847/1538-4365/ab2b9a Bibcode: 2019ApJS..243...24P

Tripp, Todd M.; Prochaska, J. Xavier; Tejos, Nicolas +10 more

We describe the survey for galaxies in the fields surrounding nine sightlines to far-UV bright, z ∼ 1 quasars that define the COS Absorption Survey of Baryon Harbors (CASBaH) program. The photometry and spectroscopy that comprise the data set come from a mixture of public surveys (SDSS, DECaLS) and our dedicated efforts on private facilities (Keck…

2019 The Astrophysical Journal Supplement Series
Gaia eHST 28
From kpcs to the central parsec of NGC 1097: feeding star formation and a black hole at the same time
DOI: 10.1093/mnras/stz579 Bibcode: 2019MNRAS.485.3264P

Bruzual, Gustavo; Burkert, Andreas; Prieto, M. Almudena +3 more

A panchromatic view of the star-forming ring and feeding process in the central kpc of the galaxy NGC 1097 is presented. The assembled IR to UV images at ∼10 pc resolution allow us to characterize the population of circa 250 clusters in the ring and disentangle the network of filaments of dust and gas that enshroud and feed them. The ring is a pla…

2019 Monthly Notices of the Royal Astronomical Society
eHST 28
LISA Pathfinder micronewton cold gas thrusters: In-flight characterization
DOI: 10.1103/PhysRevD.99.122003 Bibcode: 2019PhRvD..99l2003A

Mendes, L.; Russano, G.; Lloro, I. +76 more

The LISA Pathfinder (LPF) mission has demonstrated the ability to limit and measure the fluctuations in acceleration between two free falling test masses down to sub-femto-g levels. One of the key elements to achieve such a level of residual acceleration is the drag free control. In this scheme the spacecraft is used as a shield against any extern…

2019 Physical Review D
LISAPathfinder 28
Three-dimensional dust mapping of 12 supernovae remnants in the Galactic anticentre
DOI: 10.1093/mnras/stz1940 Bibcode: 2019MNRAS.488.3129Y

Zijlstra, A.; Jiang, B. W.; Chen, B. Q. +1 more

We present three-dimensional (3D) dust mapping of 12 supernova remnants (SNRs) in the Galactic anticentre (Galactic longitude l between 150° and 210°) based on a recent 3D interstellar extinction map. The dust distribution of the regions, which cover the full extents in the radio continuum for the individual SNRs, is discussed. Four SNRs show sign…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
An estimate of the k2 Love number of WASP-18Ab from its radial velocity measurements
DOI: 10.1051/0004-6361/201834376 Bibcode: 2019A&A...623A..45C

Csizmadia, Sz.; Smith, A. M. S.; Hellard, H.

Context. Increasing our knowledge of the interior structure, composition, and density distribution of exoplanets is crucial to make progress in the understanding of exoplanetary formation, migration and habitability. However, the directly measurable mass and radius values offer little constraint on interior structure, because the inverse problem i…

2019 Astronomy and Astrophysics
Gaia 28
Subsurface Sediment Mobilization in the Southern Chryse Planitia on Mars
DOI: 10.1029/2018JE005868 Bibcode: 2019JGRE..124..703B

Hauber, E.; Michael, G.; Brož, P. +2 more

The southern part of the smooth plain of Chryse Planitia on Mars hosts a large population of kilometer-sized (from 0.2 to 20 km) landforms spread over a wide area. Based on the investigation of a small part of this area, Komatsu et al. (2016, https://doi.org/10.1016/j.icarus.2015.12.032) p…

2019 Journal of Geophysical Research (Planets)
MEx 28
Discovery of an X-Ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524
DOI: 10.3847/1538-4357/ab4ef8 Bibcode: 2019ApJ...887...69S

Veilleux, Sylvain; Tombesi, Francesco; Lohfink, Anne M. +2 more

We present new XMM-Newton and NuSTAR observations of the galaxy merger IRAS F05189-2524, which is classified as an ultraluminous infrared galaxy and optical Seyfert 2 at z = 0.0426. We test a variety of spectral models that yield a best fit consisting of an absorbed power law with emission and absorption features in the Fe K band. Remarkably, we f…

2019 The Astrophysical Journal
XMM-Newton 28
Statistical detection of a tidal stream associated with the globular cluster M68 using Gaia data
DOI: 10.1093/mnras/stz1790 Bibcode: 2019MNRAS.488.1535P

Miralda-Escudé, Jordi; Palau, Carles G.

A method to search for tidal streams and to fit their orbits based on maximum likelihood is presented and applied to the Gaia data. Tests of the method are performed showing how a simulated stream produced by tidal stripping of a star cluster is recovered when added to a simulation of the Gaia catalogue. The method can be applied to search for str…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 28
Modeling Mg II During Solar Flares. I. Partial Frequency Redistribution, Opacity, and Coronal Irradiation
DOI: 10.3847/1538-4357/ab3c24 Bibcode: 2019ApJ...883...57K

Kerr, Graham S.; Carlsson, Mats; Allred, Joel C.

The Interface Region Imaging Spectrograph has routinely observed the flaring Mg II near-ultraviolet (NUV) spectrum, offering excellent diagnostic potential and a window into the location of energy deposition. A number of studies have forward-modeled both the general properties of these lines and specific flare observations. Generally these have fo…

2019 The Astrophysical Journal
IRIS 28
Characteristics of the Two Sequences Seen in the High-velocity Hertzsprung-Russell Diagram in Gaia DR2
DOI: 10.3847/2041-8213/ab321e Bibcode: 2019ApJ...881L..10S

Casagrande, Luca; Feltzing, Sofia; Sahlholdt, Christian L.

In this study we use a sample of about 9 million SkyMapper stars with metallicities to investigate the properties of the two stellar populations seen in the high-velocity (V T > 200 km s-1) Gaia DR2 Hertzsprung-Russell diagram. Based on 10,000 red giant branch (RGB) stars (out of 75,000 with high velocity), we find that th…

2019 The Astrophysical Journal
Gaia 28