Search Publications

On the ultra-compact nature of the neutron star system 1RXS J170854.4-321857: insights from X-ray spectroscopy
DOI: 10.1093/mnras/stz2004 Bibcode: 2019MNRAS.488.5014A

Armas Padilla, M.; López-Navas, E.

The relatively small family of ultra-compact X-ray binary systems is of great interest for many areas of astrophysics. We report on a detailed X-ray spectral study of the persistent neutron star low-mass X-ray binary 1RXS J170854.4-321857. We analysed two XMM-Newton observations obtained in late 2004 and early 2005 when, in agreement with previous…

2019 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
Searching for correlations in Gaia DR2 unbound star trajectories
DOI: 10.1093/mnras/stz2959 Bibcode: 2019MNRAS.490.5647M

García-Bellido, J.; Barrado, D.; Montanari, F.

Scattering events with compact objects are expected in the primordial black hole (PBH) cold dark matter (CDM) scenario, due to close encounters between stars and PBHs in the dense environments of dwarf spheroidals. We develop a Bayesian framework to search for correlations among Milky Way stellar trajectories and those of globular clusters and dwa…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 5
Analysis of the origin of water, carbon monoxide, and carbon dioxide in the Uranus atmosphere
DOI: 10.1051/0004-6361/201732123 Bibcode: 2019A&A...621A.129L

Lampón, M.; Lara, L. M.; Rodrigo, R. +1 more

Context. We present here an analysis of the potential sources of oxygen species in the Uranus atmosphere.
Aims: Our aim is to explain the current measurements of H2O, CO, and CO2 in the Uranus atmosphere, which would allow us to constrain the influx of oxygen-bearing species and its origin in this planet.
Methods: W…

2019 Astronomy and Astrophysics
ISO 5
How non-stationary are moderately supercritical shocks?
DOI: 10.1017/S0022377819000692 Bibcode: 2019JPlPh..85e9005G

Gedalin, Michael

Ion motion in a collisionless shock front is affected by macroscopic large-scale weakly varying and microscopic small-scale fast varying magnetic and electric fields. With the increase of the Mach number the role of the microscopic field is expected to become progressively more important. Using a combination of hybrid simulations and test particle…

2019 Journal of Plasma Physics
Cluster 5
A GALEX Far-ultraviolet Study of Dwarf Stars in Moving Groups
DOI: 10.1088/1538-3873/ab3712 Bibcode: 2019PASP..131k4201C

Smith, Graeme H.; Cochrane, Kevin M.

Far-ultraviolet (FUV) GALEX photometry of main-sequence stars in moving groups is used to verify that there is a relationship between age and FUV broadband magnitude among such stars. Samples of dwarf stars were compiled for twelve moving groups and a search made for both GALEX FUV magnitudes on the AB system and Johnson BV photometry. These data …

2019 Publications of the Astronomical Society of the Pacific
Gaia 5
Magnetic flux participation in solar surface magnetism during solar cycle 24
DOI: 10.1088/1674-4527/19/5/69 Bibcode: 2019RAA....19...69J

Wang, Jing-Xiu; Jin, Chun-Lan

This study aims at investigating surface magnetic flux participation among different types of magnetic features during solar cycle 24. State-of-the-art observations from SDO/HMI and Hinode/SOT are combined to form a unique database in the interval from April 2010 to October 2015. Unlike previous studies, the statistics presented in this paper are …

2019 Research in Astronomy and Astrophysics
Hinode 5
Generation of photoclinometric DTMs for application to transient changes on the surface of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201834127 Bibcode: 2019A&A...630A..10T

Vincent, J. -B.; Hayes, A. G.; Tang, Y. +4 more

Context. The wide spatial and temporal coverage of 67P/Churyumov-Gerasimenko (67P) by the Rosetta mission has revealed a surface created by scattered large-scale changes and numerous small-scale changes. The many small-scale changes are of particular interest because they are unexpected and ubiquitous. As their topographic relief is often smaller …

2019 Astronomy and Astrophysics
Rosetta 5
Fragmented Comet 73P/Schwassmann-Wachmann 3
DOI: 10.3847/1538-3881/ab2f7a Bibcode: 2019AJ....158..112G

Graykowski, Ariel; Jewitt, David

Comet 73P/Schwassmann-Wachmann 3 has been observed to fragment on several occasions, yet the cause of its fragmentation remains poorly understood. We use previously unpublished archival Hubble Space Telescope data taken in 2006 to study the properties of the primary fragment, 73P-C, in order to constrain the potential fragmentation mechanisms. Cur…

2019 The Astronomical Journal
eHST 5
Chemical composition of the outer halo globular cluster Palomar 15
DOI: 10.1051/0004-6361/201935467 Bibcode: 2019A&A...627A..70K

Rich, R. Michael; Xu, Siyi; Koch, Andreas

Globular clusters (GCs) in the outer Milky Way halo are important tracers of the assembly history of our Galaxy. Only a few of these objects show spreads in heavier elements beyond the canonical light-element variations that have essentially been found throughout the entire Galactic GC system, suggesting a more complex origin and evolution of thes…

2019 Astronomy and Astrophysics
Gaia 5
CN Andromedae: a shallow contact binary with a possible tertiary component
DOI: 10.1088/1674-4527/19/1/10 Bibcode: 2019RAA....19...10Y

Soydugan, Faruk; Aliçavuş, Fahri; Yildirim, Muhammed Faruk

In this study, new photometric observations of shallow contact binary CN Andromedae (CN And) were performed and multi-color (BV R) CCD light curves (LCs) were obtained. Simultaneous analysis of new LCs and published radial velocity (RV) data reveals that the system is an early contact binary in which both components have recently filled their inne…

2019 Research in Astronomy and Astrophysics
Gaia 5