Search Publications

Massive star cluster formation and evolution in tidal dwarf galaxies
DOI: 10.1051/0004-6361/201834403 Bibcode: 2019A&A...628A..60F

Weilbacher, Peter M.; Boquien, Médéric; de Grijs, Richard +8 more

Context. The formation of globular clusters remains an open debate. Dwarf starburst galaxies are efficient at forming young massive clusters with similar masses as globular clusters and may hold the key to understanding their formation.
Aims: We study star cluster formation in a tidal debris, including the vicinity of three tidal dwarf galaxi…

2019 Astronomy and Astrophysics
Gaia eHST 28
Hypotheses for the origin of the Hypanis fan-shaped deposit at the edge of the Chryse escarpment, Mars: Is it a delta?
DOI: 10.1016/j.icarus.2018.05.021 Bibcode: 2019Icar..319..885A

Sefton-Nash, Elliot; Bell, James F., III; Adler, Jacob B. +4 more

We investigated the origin of the fan-shaped deposit at the end of Hypanis Valles that has previously been proposed as an ExoMars, Mars 2020, and human mission candidate landing site, and found evidence that the landform is an ancient delta. Previous work suggests that the deposit originated from a time of fluvial activity both distinct from and p…

2019 Icarus
MEx 28
The Detection of [O III] λ4363 in a Lensed, Dwarf Galaxy at z = 2.59: Testing Metallicity Indicators and Scaling Relations at High Redshift and Low Mass
DOI: 10.3847/1538-4357/ab5713 Bibcode: 2019ApJ...887..168G

Richard, Johan; Siana, Brian; Freeman, William R. +6 more

We present Keck/MOSFIRE (Multi-Object Spectrometer for InfraRed Exploration) and Keck/LRIS (Low Resolution Imaging Spectrometer) spectroscopy of A1689-217, a lensed (magnification ∼7.9), star-forming (SFR ∼ 16 M yr-1), dwarf (log(M */M ) = 8.07-8.59) Lyα emitter (EW0 ∼ 138 Å) at z = 2.5918.…

2019 The Astrophysical Journal
eHST 28
The solar chromosphere at millimetre and ultraviolet wavelengths. I. Radiation temperatures and a detailed comparison
DOI: 10.1051/0004-6361/201834205 Bibcode: 2019A&A...622A.150J

De Pontieu, B.; Rezaei, R.; Carlsson, M. +3 more

Solar observations with the Atacama Large Millimeter/submillimeter Array (ALMA) provide us with direct measurements of the brightness temperature in the solar chromosphere. We study the temperature distributions obtained with ALMA Band 6 (in four sub-bands at 1.21, 1.22, 1.29, and 1.3 mm) for various areas at, and in the vicinity of, a sunspot, co…

2019 Astronomy and Astrophysics
IRIS 28
Simulations of Ice Chemistry in Cometary Nuclei
DOI: 10.3847/1538-4357/ab418e Bibcode: 2019ApJ...884...69G

Garrod, Robin T.

The first computational model of solid-phase chemistry in cometary nuclear ices is presented. An astrochemical kinetics model, the Model for Astrophysical Gas and Ice Chemical Kinetics And Layering, is adapted to trace the chemical evolution in multiple layers of cometary ice, over a representative period of 5 Gyr. Physical conditions are chosen a…

2019 The Astrophysical Journal
Rosetta 28
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