Search Publications

MUSE spectroscopy of the ULX NGC 1313 X-1: A shock-ionised bubble, an X-ray photoionised nebula, and two supernova remnants
DOI: 10.1051/0004-6361/202142229 Bibcode: 2022A&A...666A.100G

Godet, O.; Contini, T.; Olive, J. -F. +2 more

Context. The presence of large ionised gaseous nebulae found around some ultraluminous X-ray sources (ULXs) provides the means to assess the mechanical and radiative feedback of the central source, and hence constrain the efficiency and impact on the surroundings of the super-Eddington regime powering most of these sources. NGC 1313 X-1 is an arch…

2022 Astronomy and Astrophysics
Gaia eHST 23
wdwarfdate: A Python Package to Derive Bayesian Ages of White Dwarfs
DOI: 10.3847/1538-3881/ac7788 Bibcode: 2022AJ....164...62K

Angus, Ruth; Kiman, Rocio; Xu, Siyi +5 more

White dwarfs have been successfully used as cosmochronometers in the literature; however, their reach has been limited in comparison to their potential. We present wdwarfdate, a publicly available Python package to derive the Bayesian age of a white dwarf, based on its effective temperature (T eff) and surface gravity (log g). We make t…

2022 The Astronomical Journal
Gaia 23
The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and γ-rays
DOI: 10.1093/mnras/stac1440 Bibcode: 2022MNRAS.514.2239S

Strader, Jay; Chomiuk, Laura; Ness, Jan-Uwe +16 more

Peaking at 3.7 mag on 2020 July 11, YZ Ret was the second-brightest nova of the decade. The nova's moderate proximity (2.7 kpc, from Gaia) provided an opportunity to explore its multiwavelength properties in great detail. Here, we report on YZ Ret as part of a long-term project to identify the physical mechanisms responsible for high-energy emissi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 23
The Gaia EDR3 view of Johnson-Kron-Cousins standard stars: the curated Landolt and Stetson collections
DOI: 10.1051/0004-6361/202243939 Bibcode: 2022A&A...664A.109P

Rainer, M.; Marinoni, S.; Marrese, P. M. +7 more

Context. In the era of large surveys and space missions, it is necessary to rely on large samples of well-characterized stars for inter-calibrating and comparing measurements from different surveys and catalogues. Among the most employed photometric systems, the Johnson-Kron-Cousins has been used for decades and for a large amount of important dat…

2022 Astronomy and Astrophysics
Gaia Hipparcos 23
The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo
DOI: 10.1093/mnrasl/slac126 Bibcode: 2022MNRAS.517L.138O

Springel, Volker; Orkney, Matthew D. A.; Laporte, Chervin F. P. +6 more

We identify and characterize a Milky Way-like realization from the Auriga simulations with two consecutive massive mergers $\sim 2$ Gyr apart at high redshift, comparable to the reported Kraken and Gaia-Sausage-Enceladus. The Kraken-like merger (z = 1.6, $M_{\rm Tot}=8\times 10^{10}\, \rm {M_{\odot }}$) is gas-rich, deposits most of its mass in th…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 23
LISC Catalog of Star Clusters. I. Galactic Disk Clusters in Gaia EDR3
DOI: 10.3847/1538-4365/ac3c49 Bibcode: 2022ApJS..259...19L

Li, Zhongmu; Liu, Xuejie; Chen, Wen +6 more

This work searches for the candidates of Galactic disk star clusters in Gaia Early Data Release 3 (Gaia EDR3) and determines their basic parameters from color-magnitude diagrams (CMDs). A friends-of-friends method for membership determination and stellar population models including binary stars (ASPS) and rotating stars are adopted. As a result, 8…

2022 The Astrophysical Journal Supplement Series
Gaia 23
Insight-HXMT, NuSTAR, and INTEGRAL Data Show Disk Truncation in the Hard State of the Black Hole X-Ray Binary MAXI J1820+070
DOI: 10.3847/1538-4357/ac54a7 Bibcode: 2022ApJ...928...11Z

Zdziarski, Andrzej A.; You, Bei; Szanecki, Michał +2 more

We study X-ray and soft gamma-ray spectra from the hard state of the accreting black hole binary MAXI J1820+070. We perform an analysis of joint spectra from HXMT, NuSTAR, and INTEGRAL. We find an overall agreement between the spectra from all three satellites. Satisfactory fits to the data require substantial spectral complexity, with our models …

2022 The Astrophysical Journal
INTEGRAL 23
Gaia spectroscopic orbits validated with LAMOST and GALAH radial velocities
DOI: 10.1093/mnras/stac2928 Bibcode: 2022MNRAS.517.3888B

Mazeh, T.; Faigler, S.; Jorissen, A. +5 more

The recently published Gaia DR3 catalogue of $181\, 327$ spectroscopic binaries (SB) includes the Keplerian elements of each orbit but not the measured radial velocities (RVs) and their epochs. Instead, the catalogue lists a few parameters that characterize the robustness of each solution. In this work, we use two external sources to validate the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 23
The Deuterium Isotopic Ratio of Water Released From the Martian Caps as Measured With TGO/NOMAD
DOI: 10.1029/2022GL098161 Bibcode: 2022GeoRL..4998161V

Vandaele, Ann Carine; Brines, Adrian; Aoki, Shohei +18 more

We report vertical profiles of water and D/H for one Martian year as measured with the TGO/NOMAD instrument. The observations were performed via solar occultation, providing water profiles up to ∼100 km and D/H up to ∼60 km, with a vertical resolution of 1-2 km. The measurements reveal dramatic variability of water and D/H over short timescales an…

2022 Geophysical Research Letters
ExoMars-16 23
A dynamically discovered and characterized non-accreting neutron star-M dwarf binary candidate
DOI: 10.1038/s41550-022-01766-0 Bibcode: 2022NatAs...6.1203Y

Huang, Yang; Liu, Jifeng; Bai, Yu +26 more

Typically, neutron stars are discovered by observations at radio, X-ray or gamma-ray wavelengths. Unlike radio pulsar surveys and X-ray observations, optical time-domain surveys can unveil and characterize exciting but less explored non-accreting and/or non-beaming neutron stars in binaries. Here we report the discovery of such a neutron star cand…

2022 Nature Astronomy
Gaia IUE 23