Search Publications

Ultraviolet and X-ray properties of Coma's ultra-diffuse galaxies
DOI: 10.1093/mnras/staa1955 Bibcode: 2020MNRAS.497.2759L

Gallo, Elena; Hodges-Kluck, Edmund; Lee, Chris H.

Many ultra-diffuse galaxies (UDGs) have been discovered in the Coma cluster, and there is evidence that some, notably Dragonfly 44, have Milky Way-like dynamical masses despite dwarf-like stellar masses. We used X-ray, ultraviolet (UV), and optical data to investigate the star formation and nuclear activity in the Coma UDGs, and we obtained deep U…

2020 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 8
The historical record of massive star formation in Cygnus
DOI: 10.1051/0004-6361/202039188 Bibcode: 2020A&A...644A..62C

Comerón, F.; Schneider, N.; Pasquali, A. +1 more

Context. The Cygnus region, which dominates the local spiral arm of the Galaxy, is one of the nearest complexes of massive star formation, extending over several hundred parsecs. Its massive stellar content, regions of ongoing star formation, and molecular gas have been studied in detail at virtually all wavelengths. However, little is known of th…

2020 Astronomy and Astrophysics
Gaia 8
A Non-Linear Magnetic Field Calibration Method for Filter-Based Magnetographs by Multilayer Perceptron
DOI: 10.1007/s11207-019-1573-9 Bibcode: 2020SoPh..295....5G

Ji, Kaifan; Su, Jiangtao; Deng, Yuanyong +5 more

For filter-based magnetographs, the linear calibration method under the weak-field assumption is usually adopted; this leads to magnetic saturation effect in the regions with strong magnetic field. This article explores a new method to overcome the above disadvantage using a multilayer perceptron network, which we call MagMLP, based on a back-prop…

2020 Solar Physics
Hinode 8
Mapping and spatial statistical analysis of Mars Yardangs
DOI: 10.1016/j.pss.2020.105035 Bibcode: 2020P&SS..19205035L

Di, Kaichang; Liu, Bin; Liu, Jia +4 more

Mars yardang fields were mapped using the newly available high-resolution Context Camera (CTX) mosaics (30°N to 30°S) through visual interpretation and manual digitization. We classified the Martian yardangs into three types according to their shapes: long ridge, inverted hull and curvilinear shapes, and found that the number of long ridge yardang…

2020 Planetary and Space Science
MEx 8
Space debris observations with the Slovak AGO70 telescope: Astrometry and light curves
DOI: 10.1016/j.asr.2020.01.038 Bibcode: 2020AdSpR..65.2018S

Šilha, Jiří; Krajčovič, Stanislav; Zigo, Matej +12 more

The Faculty of Mathematics, Physics and Informatics of Comenius University in Bratislava, Slovakia (FMPI) operates its own 0.7-m Newtonian telescope (AGO70) dedicated to the space surveillance tracking and research, with an emphasis on space debris. The observation planning focuses on objects on geosynchronous (GEO), eccentric (GTO and Molniya) an…

2020 Advances in Space Research
Gaia 8
Do bulges stop stars forming?
DOI: 10.1093/mnras/stz2971 Bibcode: 2020MNRAS.491...69E

Eales, Stephen; Eales, Oliver; de Vis, Pieter

In this paper, we use the Herschel Reference Survey to make a direct test of the hypothesis that the growth of a stellar bulge leads to a reduction in the star formation efficiency of a galaxy (or conversely a growth in the gas-depletion time-scale) as a result of the stabilization of the gaseous disc by the gravitational field of the bulge. We fi…

2020 Monthly Notices of the Royal Astronomical Society
Herschel 8
Sporadic and intense accretion in a 1 Myr-old brown dwarf candidate
DOI: 10.1051/0004-6361/201936810 Bibcode: 2020A&A...634A.128N

Bessell, M. S.; Murphy, S. J.; Nguyen-Thanh, D. +1 more

Context. Studying the accretion process in very low-mass objects has important implications for understanding their formation mechanism. Many nearby late-M dwarfs that have previously been identified in the field are in fact young brown dwarf members of nearby young associations. Some of them are still accreting. They are therefore excellent targe…

2020 Astronomy and Astrophysics
Gaia 8
Dynamical Mass Estimates of the β Pictoris Planetary System through Gaussian Process Stellar Activity Modeling
DOI: 10.3847/1538-3881/abba30 Bibcode: 2020AJ....160..243V

Vandal, Thomas; Doyon, René; Rameau, Julien

Nearly 15 yr of radial velocity (RV) monitoring and direct imaging enabled the detection of two giant planets orbiting the young, nearby star β Pictoris. The δ Scuti pulsations of the star, which overwhelm planetary signals, need to be carefully suppressed. In this work, we independently revisit the analysis of the RV data following a different ap…

2020 The Astronomical Journal
Gaia 8
The nature of the symbiotic candidate 2MASS J07363415+6538548 in the field of NGC 2403
DOI: 10.1093/mnras/staa3063 Bibcode: 2020MNRAS.499.2116M

Merc, J.; Gális, R.; Wolf, M. +2 more

New Online Database of Symbiotic Variables includes several poorly characterized objects and candidate symbiotic stars, not only in the Milky Way but also in other galaxies. The goal of the research presented in this paper was to reveal the nature of 2MASS J07363415+6538548, the object discovered as an X-ray source in the field of NGC 2403, and te…

2020 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton eHST 8
Determining the origin of the building blocks of the Ice Giants based on analogue measurements from comets
DOI: 10.1093/mnras/stz3061 Bibcode: 2020MNRAS.491..488M

Mousis, O.; Mandt, K. E.; Treat, S.

The abundances of the heavy elements and isotopic ratios in the present atmospheres of the giant planets can be used to trace the composition of volatiles that were present in the icy solid material that contributed to their formation. The first definitive measurements of noble gas abundances and isotope ratios at comet 67P/Churyumov-Gerasimenko (…

2020 Monthly Notices of the Royal Astronomical Society
Rosetta 8