Search Publications

The phenomenon of shape evolution from solar-driven outgassing for analogues of small Kuiper belt objects
DOI: 10.1093/mnras/staa132 Bibcode: 2020MNRAS.492.5152Z

Rezac, L.; Li, J. -Y.; Zhao, Y. +1 more

One of the key findings of the Rosetta mission to the Jupiter-family comet 67P/Churyumov-Gerasimenko was its peculiar bi-lobed shape and its apparent Northern/Southern hemispheric dichotomy in large-scale morphology. This has re-ignited scientific discussions on the topic of the origin, evolution and age of the nucleus. In this work, we conduct a …

2020 Monthly Notices of the Royal Astronomical Society
Rosetta 6
Onthe changes in the physical properties of the ionized region around the Weigelt structures in η Carinae over the 5.54-yr spectroscopic cycle
DOI: 10.1093/mnras/staa1311 Bibcode: 2020MNRAS.495.2754T

Gull, T. R.; Corcoran, M. F.; Hillier, D. J. +3 more

We present HST/STIS observations and analysis of two prominent nebular structures around the central source of η Carinae, the knots C and D. The former is brighter than the latter for emission lines from intermediate- or high-ionization potential ions. The brightness of lines from intermediate- and high-ionization potential ions significantly decr…

2020 Monthly Notices of the Royal Astronomical Society
eHST 6
Pulsation in the white dwarf HE 1017-1352: confirmation of the class of hot DAV stars
DOI: 10.1093/mnrasl/slaa106 Bibcode: 2020MNRAS.497L..24R

Kepler, S. O.; Romero, Alejandra D.; Antunes Amaral, L. +3 more

We report the detection of periodic variations on the $T_\mathrm{eff}\simeq 32\, 000$ K DA white dwarf star HE 1017-1352. We obtained time series photometry using the 4.1-m Southern Astrophysical Research telescope on three separate nights for a total of 16.8 h. From the frequency analysis, we found four periods of 605, 556, 508, and 869 s with si…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
A low-mass stellar companion to the young variable star RZ Psc
DOI: 10.1093/mnrasl/slaa092 Bibcode: 2020MNRAS.496L..75K

Henning, Thomas; Ménard, François; Kral, Quentin +10 more

RZ Psc is a young Sun-like star with a bright and warm infrared excess that is occasionally dimmed significantly by circumstellar dust structures. Optical depth arguments suggest that the dimming events do not probe a typical sightline through the circumstellar dust, and are instead caused by structures that appear above an optically thick mid-pla…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
Luminous blue variable candidates in M31
DOI: 10.1093/mnras/staa1729 Bibcode: 2020MNRAS.497..687S

Vinokurov, A.; Solovyeva, Y.; Bizyaev, D. +7 more

We study five luminous blue variable (LBV) candidates in the Andromeda galaxy and one more (MN112) in the Milky Way. We obtain the same-epoch near-infrared (NIR) and optical spectra on the 3.5-m telescope at the Apache Point Observatory and on the 6-m telescope of the SAO RAS. The candidates show typical LBV features in their spectra: broad and st…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
Searching for eclipsing binaries in the area of RA: 02h21m36s, Dec: +5711'32″
DOI: 10.1093/mnras/staa2170 Bibcode: 2020MNRAS.497.3381G

Li, Kai; Gao, Xing; Sun, Guo-You +5 more

By analysing the data observed by the Comet Search Programme telescope at Xingming Observatory from 2018 October 11 to 2018 December 19, 24 eclipsing binaries were identified. By cross-matching with the VSX (AAVSO) website, we found that four binaries are newly discovered. By analysing the Transiting Exoplanet Survey Satellite (TESS) data, the lig…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
Kinematics of main-sequence stars from the Gaia DR2 and PMA proper motions
DOI: 10.1093/mnras/staa825 Bibcode: 2020MNRAS.494.1430V

Akhmetov, V. S.; Fedorov, P. N.; Velichko, Anna B.

We aim at analysis of kinematics of main-sequence stars from the GaiaDR2 and PMA catalogues as well as comparison of kinematic parameters derived from their proper motions. We decompose the stellar velocity field on to a set of vector spherical harmonics (VSH), and, using the relations between the decomposition coefficients and the Ogorodnikov-Mil…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
AStroLens: automatic strong-lens modelling of X-ray selected galaxy clusters
DOI: 10.1093/mnras/staa2180 Bibcode: 2020MNRAS.498.1121Z

Ebeling, Harald; Zalesky, Lukas

We use AStroLens, a newly developed gravitational lens-modelling code that relies only on geometric and photometric information of cluster galaxies as input, to map the strong-lensing regions and estimate the lensing strength of 96 galaxy clusters at z = 0.5-0.9. All clusters were identified during the extended Massive Cluster Survey (eMACS) based…

2020 Monthly Notices of the Royal Astronomical Society
eHST 6
A Swift view of X-ray and UV radiation in the planet-forming T Tauri system PDS 70
DOI: 10.1093/mnrasl/slz169 Bibcode: 2020MNRAS.491L..56J

Güdel, Manuel; Pye, John P.; Page, Kim L. +4 more

PDS 70 is a ∼5-Myr-old star with a gas and dust disc in which several protoplanets have been discovered. We present the first ultraviolet (UV) detection of the system along with X-ray observations taken with the Neil Gehrels Swift Observatory satellite. PDS 70 has an X-ray flux of 3.4 × 10-13 erg cm-2 s-1 in the 0.…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 6
Structural parameters for the globular-cluster-like objects in NGC 1052-DF2
DOI: 10.1093/mnras/staa1775 Bibcode: 2020MNRAS.496.3741M

Zou, Hu; Nie, Jundan; Zhang, Tianmeng +8 more

Recently, van Dokkum et al. have found an ultra-diffuse galaxy NGC 1052-DF2 with little or no dark matter, based on a spectroscopic study of its 11 constituent globular-cluster-like objects. In this paper, we analyse these 11 objects using Hubble Space Telescope imaging. We derive the structural parameters for each object by fitting the surface br…

2020 Monthly Notices of the Royal Astronomical Society
eHST 6