Search Publications

Neutron-capture elements record the ordered chemical evolution of the disc over time
DOI: 10.1093/mnras/stac953 Bibcode: 2022MNRAS.513.5477H

Buder, Sven; Ness, Melissa K.; Horta, Danny +2 more

An ensemble of chemical abundances probing different nucleosynthetic channels can be leveraged to build a comprehensive understanding of the chemical and structural evolution of the Galaxy. Using GALAH DR3 data, we seek to trace the enrichment by the supernovae Ia, supernovae II, asymptotic giant branch stars, and neutron-star mergers and/or colla…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Serendipitous discovery of radio flaring behaviour from a nearby M dwarf with MeerKAT
DOI: 10.1093/mnras/stac1002 Bibcode: 2022MNRAS.513.3482A

Buckley, David A. H.; Osten, Rachel A.; Lintott, Chris J. +12 more

We report on the detection of MKT J174641.0-321404, a new radio transient found in untargeted searches of wide-field MeerKAT radio images centred on the black hole X-ray binary H1743-322. MKT J174641.0-321404 is highly variable at 1.3 GHz and was detected three times during 11 observations of the field in late 2018, reaching a maximum flux density…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Thermal and non-thermal X-ray emission from the rotation-powered radio/γ-ray pulsar PSR J1740+1000
DOI: 10.1093/mnras/stac1130 Bibcode: 2022MNRAS.513.3113R

Mereghetti, Sandro; Turolla, Roberto; Zane, Silvia +4 more

We report the results of new XMM-Newton observations of the middle-aged (τc = 1.1 × 105 yr) radio pulsar PSR J1740+1000 carried out in 2017-2018. These long pointings (~530 ks) show that the non-thermal emission, well described by a power-law spectrum with photon index Γ = 1.80 ± 0.17, is pulsed with a ~30 per cent pulsed fra…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 15
WISDOM Project - XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
DOI: 10.1093/mnras/stac2493 Bibcode: 2022MNRAS.516.4066L

Williams, Thomas G.; Cappellari, Michele; Davis, Timothy A. +5 more

The mm-Wave Interferometric Survey of Dark Object Masses (WISDOM) is probing supermassive black holes (SMBHs) in galaxies across the Hubble sequence via molecular gas dynamics. We present the first WISDOM study of a luminous infrared galaxy with an active galactic nuclei (AGNs): Fairall 49. We use new ALMA observations of the CO(2 - 1) line with a…

2022 Monthly Notices of the Royal Astronomical Society
eHST 15
Mass transfer and tidally tilted pulsation in the Algol-type system TZ Dra
DOI: 10.1093/mnras/stab3515 Bibcode: 2022MNRAS.510.1413K

Handler, G.; Leone, F.; De Cat, P. +6 more

Oscillating eclipsing Algols (oEAs) are remarkable systems that allow us to determine accurate fundamental stellar parameters (mass, radius) and probe the stellar interiors through pulsations. TZ Dra is an oEA system containing a δ Scuti component. To examine particular characteristics of such close systems including pulsations and mass transfer, …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
Still at odds with conventional galaxy evolution: the star formation history of ultradiffuse galaxy Dragonfly 44
DOI: 10.1093/mnras/stac2417 Bibcode: 2022MNRAS.516.3318W

van Dokkum, Pieter; Forbes, Duncan A.; Romanowsky, Aaron J. +7 more

We study the star formation history (SFH) of the ultradiffuse galaxy (UDG) Dragonfly 44 (DF44) based on the simultaneous fit to near-ultraviolet to near-infrared photometry and high signal-to-noise optical spectroscopy. In fitting the observations, we adopt an advanced physical model with a flexible SFH and discuss the results in the context of th…

2022 Monthly Notices of the Royal Astronomical Society
eHST 15
Planetary nebulae with Wolf-Rayet-type central stars - III. A detailed view of NGC 6905 and its central star
DOI: 10.1093/mnras/stab3042 Bibcode: 2022MNRAS.509..974G

Guerrero, M. A.; Toalá, J. A.; Todt, H. +6 more

We present a multiwavelength characterization of the planetary nebula (PN) NGC 6905 and its [Wolf-Rayet]-type ([WR]) central star (CSPN) HD 193949. Our Nordic Optical Telescope Alhambra Faint Object Spectrograph and Camera (ALFOSC) spectra and images unveil in unprecedented detail the high-ionization structure of NGC 6905. The high-quality spectra…

2022 Monthly Notices of the Royal Astronomical Society
AKARI Gaia eHST 15
Spectral analysis of cool white dwarfs accreting from planetary systems: from the ultraviolet to the optical
DOI: 10.1093/mnras/stab3696 Bibcode: 2022MNRAS.511...71H

Gänsicke, B. T.; Tremblay, P. -E.; Hollands, M. A. +1 more

The accretion of planetary debris into the atmospheres of white dwarfs leads to the presence of metal lines in their spectra. Cool metal-rich white dwarfs, which left the main sequence many Gyr ago, allow the study of the remnants of the oldest planetary systems. Despite their low effective temperatures (Teff), a non-negligible amount o…

2022 Monthly Notices of the Royal Astronomical Society
eHST 15
Filling the gap between synchronized and non-synchronized sdBs in short-period sdBV+dM binaries with TESS: TIC 137608661, a new system with a well-defined rotational splitting
DOI: 10.1093/mnras/stac160 Bibcode: 2022MNRAS.511.2201S

Németh, Péter; Silvotti, Roberto; Telting, John H. +5 more

TIC 137608661/TYC 4544-2658-1/FBS 0938+788 is a new sdBV+dM reflection-effect binary discovered by the TESS space mission with an orbital period of 7.21 h. In addition to the orbital frequency and its harmonics, the Fourier transform of TIC 137608661 shows many g-mode pulsation frequencies from the subdwarf B (sdB) star. The amplitude spectrum is …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15
The nova KT Eri Is a recurrent nova with a recurrence time-scale of 40-50 yr
DOI: 10.1093/mnras/stac2923 Bibcode: 2022MNRAS.517.3864S

Walter, Frederick M.; Schaefer, Bradley E.; Hounsell, Rebekah +1 more

KT Eridani was a very fast nova in 2009 peaking at V = 5.42 mag. We marshal large data sets of photometry to finally work out the nature of KT Eri. From the TESS light curve, as confirmed with our radial velocity curve, we find an orbital period of 2.61595 d. With our 272 spectral energy distributions from simultaneous BVRIJHK measures, the compan…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 15