Search Publications

Sizing from the smallest scales: the mass of the Milky Way
DOI: 10.1093/mnras/stac1265 Bibcode: 2022MNRAS.513.4968R

Cooper, M. C.; Simon, J. D.; Ji, A. P. +6 more

As the Milky Way and its satellite system become more entrenched in near field cosmology efforts, the need for an accurate mass estimate of the Milky Way's dark matter halo is increasingly critical. With the second and early third data releases of stellar proper motions from Gaia, several groups calculated full 6D phase-space information for the p…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Asteroseismology of the double-radial mode δ Scuti star BP Pegasi
DOI: 10.1093/mnras/stac646 Bibcode: 2022MNRAS.512.3551D

Daszyńska-Daszkiewicz, J.; Pamyatnykh, A. A.; Walczak, P. +1 more

Using the All-Sky Automated Survey data, we determine the pulsational frequencies of the high-amplitude δ Scuti star BP Pegasi. The analysis revealed only the two known, independent frequencies that we use to perform the seismic analysis of the star. On the basis of multicolour Strömgren photometry, we independently find that both frequencies can …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Globular Cluster UVIT Legacy Survey (GlobULeS) - I. FUV-optical colour-magnitude diagrams for eight globular clusters
DOI: 10.1093/mnras/stac1209 Bibcode: 2022MNRAS.514.1122S

Dalessandro, Emanuele; Hutchings, John; Stetson, Peter B. +22 more

We present the first results of eight globular clusters (GCs) from the AstroSat/UVIT Legacy Survey programme GlobULeS based on the observations carried out in two far-ultraviolet (FUV) filters (F148W and F169M). The FUV-optical and FUV-FUV colour-magnitude diagrams (CMDs) of GCs with the proper motion membership were constructed by combining the U…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 13
Candidate isolated neutron stars in the 4XMM-DR10 catalogue of X-ray sources
DOI: 10.1093/mnras/stab2974 Bibcode: 2022MNRAS.509.1217R

Mereghetti, Sandro; Rigoselli, Michela; Tresoldi, Caterina

Most isolated neutron stars have been discovered thanks to the detection of their pulsed non-thermal emission, at wavelengths spanning from radio to gamma-rays. However, if the beamed non-thermal radiation does not intercept our line of sight or it is too faint or absent, isolated neutron stars can also be detected through their thermal emission, …

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 13
Multicomponent DHOST analysis in galaxy clusters
DOI: 10.1093/mnras/stac180 Bibcode: 2022MNRAS.511.1878L

Umetsu, Keiichi; Salzano, Vincenzo; Laudato, Enrico

Extended theories of gravity with additional scalar degrees of freedom have recently acquired increasing interest due to the presence of a screening mechanism that allows suppressing at small scales (e.g. the Solar system scale) every modification restoring general relativity (GR). In this work, we consider a second-order extended theory of gravit…

2022 Monthly Notices of the Royal Astronomical Society
eHST 13
7Be in the outburst of the ONe nova V6595 Sgr
DOI: 10.1093/mnras/stab3106 Bibcode: 2022MNRAS.509.3258M

Bonifacio, P.; Hernanz, M.; D'Odorico, V. +7 more

We report on the search for the 7Be II isotope in the outbursts of the classical nova V6595 Sgr by means of high-resolution Ultraviolet and Visual Echelle Spectrograph (UVES) observations taken at the European Southern Observatory's Very Large Telescope in 2021 April, about two weeks after its discovery and under difficult circumstances…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
The formation of the Milky Way halo and its dwarf satellites: A NLTE-1D abundance analysis. V. The Sextans galaxy
DOI: 10.1093/mnras/stab3189 Bibcode: 2022MNRAS.509.3626M

Jablonka, P.; Yakovleva, S. A.; Belyaev, A. K. +3 more

We present a homogeneous set of accurate atmospheric parameters for a sample of eleven very metal-poor (-3.32 ≤ [Fe/H] ≤-2.61) stars in the Sextans dwarf spheroidal galaxy (dSph) and the non-local thermodynamic equilibrium (NLTE) abundances of, at least, seven chemical elements based on high-resolution UVES/VLT and HDS/Subaru spectra. For each sta…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
The family pictures of our neighbours: investigating the mass function and dynamical parameters of nearby open clusters
DOI: 10.1093/mnras/stac2562 Bibcode: 2022MNRAS.516.5637E

Sollima, A.; Haghi, H.; Ebrahimi, H.

We determine the mass functions (MFs) and the dynamical parameters of 15 nearby open clusters (OCs), using the unprecedented data set of the Gaia Early Data Release 3. We select the members of each cluster by combining the photometric (colour and magnitude) and astrometric (parallax and proper motions) parameters of stars, minimizing the contamina…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Project Hephaistos - I. Upper limits on partial Dyson spheres in the Milky Way
DOI: 10.1093/mnras/stac280 Bibcode: 2022MNRAS.512.2988S

Wright, Jason T.; Zackrisson, Erik; Korn, Andreas J. +2 more

Dyson spheres are hypothetical megastructures built by advanced extraterrestrial civilizations to harvest radiation energy from stars. Here, we combine optical data from Gaia DR2 with mid-infrared data from AllWISE to set the strongest upper limits to date on the prevalence of partial Dyson spheres within the Milky Way, based on their expected was…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
The stellar 'Snake' - I. Whole structure and properties
DOI: 10.1093/mnras/stac843 Bibcode: 2022MNRAS.513..503W

Fang, Min; Wang, Fan; Tian, Haijun +10 more

To complement our previous discovery of the young snake-like structure in the solar neighbourhood and reveal the structure's full extent, we build two samples of stars within the Snake and its surrounding territory from Gaia Early Data Release 3 (EDR3). With the friends-of-friends algorithm, we identify 2694 and 9052 Snake member candidates from t…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13