Search Publications

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
Evolution of exploding granules from coordinated observations by THEMIS, IRIS, SDO/HMI, and HINODE, and a simulation
DOI: 10.1051/0004-6361/202038132 Bibcode: 2020A&A...641A..50R

Malherbe, J. M.; Dalmasse, K.; Roudier, T. +3 more

Exploding granules constitute the strongest horizontal flows on the quiet Sun and contribute to the structure of the surface horizontal velocity fields which build the large-scale organization of the discrete magnetic field. In this work we explore exploding granule expansion through the observations of the ground-based THEMIS telescope, IRIS, SDO…

2020 Astronomy and Astrophysics
Hinode IRIS 8
How to disentangle geometry and mass-loss rate from AGB-star spectral energy distributions. The case of EP Aquarii
DOI: 10.1051/0004-6361/202038029 Bibcode: 2020A&A...642A.142W

Jorissen, A.; Decin, L.; Groenewegen, M. A. T. +2 more

Context. High-angular-resolution observations of asymptotic giant branch (AGB) stars often reveal non-spherical morphologies for the gas and dust envelopes.
Aims: We aim to make a pilot study to quantify the impact of different geometries (spherically symmetric, spiral-shaped, and disc-shaped) of the dust component of AGB envelopes on spectra…

2020 Astronomy and Astrophysics
Gaia Herschel ISO 8
K2-HERMES II. Planet-candidate properties from K2 Campaigns 1-13
DOI: 10.1093/mnras/staa1528 Bibcode: 2020MNRAS.496..851W

Kane, Stephen R.; Casey, Andrew R.; Wittenmyer, Robert A. +22 more

Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host star in as much detail as possible. We present complete results for planet-candidate hosts from the K2-HERMES survey, which uses the HERMES multi-object spectrograph on…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 8
The Kasei Valles, Mars: a unified record of episodic channel flows and ancient ocean levels
DOI: 10.1038/s41598-020-75080-y Bibcode: 2020NatSR..1018571D

Duran, Sergio; Coulthard, Tom J.

There is widespread evidence across Mars of past flows in major channel systems as well as more than one palaeo ocean level. However, evidence for the timing of channel flows and ocean levels is based on geographically diverse sources with a limited number of dates, making reconstructions of palaeo flows and ocean levels patchy. Here, based on hig…

2020 Scientific Reports
MEx 8