Search Publications

Offset of M54 from the Sagittarius dwarf spheroidal galaxy
DOI: 10.1093/mnras/stae1680 Bibcode: 2024MNRAS.532.3713A

Pace, Andrew B.; Walker, Matthew G.; An, Zhaozhou

We present results from simultaneous modelling of 2D (projected along the line of sight) position, proper motion, and line-of-sight velocity for Gaia- and Apache Point Observatory Galactic Evolution Experiment (APOGEE)-observed stars near the centre of the Sagittarius (Sgr) dwarf spheroidal galaxy. We use a mixture model that allows for independen…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Constraints on the ultra-high energy cosmic ray output of gamma-ray bursts
DOI: 10.1093/mnras/stae873 Bibcode: 2024MNRAS.530..555M

Gendre, B.; Orange, N. B.; Moore, E. +1 more

Ultra-high energy cosmic rays are the most extreme energetic particles detected on Earth, however, their acceleration sites are still mysterious. We explore the contribution of low-luminosity gamma-ray bursts to the ultra-high energy cosmic ray flux, since they form the bulk of the nearby population. We analyse a representative sample of these bur…

2024 Monthly Notices of the Royal Astronomical Society
INTEGRAL 2
Structure and dynamics of the Hermean magnetosphere revealed by electron observations from the Mercury electron analyzer after the first three Mercury flybys of BepiColombo
DOI: 10.1051/0004-6361/202449450 Bibcode: 2024A&A...687A.243R

André, N.; Fedorov, A.; Sauvaud, J. -A. +16 more

Context. The Mercury electron analyzer (MEA) obtained new electron observations during the first three Mercury flybys by BepiColombo on October 1, 2021 (MFB1), June 23 , 2022 (MFB2), and June 19, 2023 (MFB3). BepiColombo entered the dusk side magnetotail from the flank magnetosheath in the northern hemisphere, crossed the Mercury solar orbital equ…

2024 Astronomy and Astrophysics
BepiColombo 2
Discovery of Astrometric Accelerations by Dark Companions in the Globular Cluster ω Centauri
DOI: 10.3847/1538-4357/ad167c Bibcode: 2024ApJ...963...60P

Kamann, Sebastian; Girardi, Léo; Kozhurina-Platais, Vera +6 more

We present results from the search for astrometric accelerations of stars in ω Centauri using 13 yr of regularly scheduled Hubble Space Telescope WFC3/UVIS calibration observations in the cluster core. The high-precision astrometry of ∼160,000 sources was searched for significant deviations from linear proper motion. This led to the discovery of f…

2024 The Astrophysical Journal
Gaia eHST 2
A combined LOFAR and XMM-Newton analysis of the disturbed cluster PSZ2G113.91-37.01
DOI: 10.1051/0004-6361/202346591 Bibcode: 2024A&A...683A...9C

Brunetti, G.; Rossetti, M.; Gastaldello, F. +10 more

In this work, we investigate the interplay between the X-ray and radio emission of the cluster PSZ2G113.91-37.01 (z = 0.371) using the high-quality XMM-Newton observations of the Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of structure formation (CHEX-MATE), and the images from the second data releas…

2024 Astronomy and Astrophysics
XMM-Newton 2
A Long-duration Superflare on the K Giant HD 251108
DOI: 10.3847/1538-4357/ad8b2c Bibcode: 2024ApJ...977....6G

Schmitt, J. H. M. M.; Notsu, Yuta; Maehara, Hiroyuki +10 more

Many giant stars are magnetically active, which causes rotational variability, chromospheric emission lines, and X-ray emission. Large outbursts in these emission features can set limits on the magnetic field strength and thus constrain the mechanism of the underlying dynamo. HD 251108 is a Li-rich active K-type giant. We find a rotational period …

2024 The Astrophysical Journal
Gaia XMM-Newton 2
Time Series of Magnetic Field Parameters of Merged MDI and HMI Space-weather Active Region Patches as Potential Tool for Solar Flare Forecasting
DOI: 10.3847/1538-4357/ad60c3 Bibcode: 2024ApJ...972..169K

Kosovichev, Alexander G.; Nita, Gelu M.; Sadykov, Viacheslav M. +8 more

Solar flare prediction studies have been recently conducted with the use of Space-Weather MDI (Michelson Doppler Imager on board Solar and Heliospheric Observatory) Active Region Patches (SMARPs) and Space-Weather HMI (Helioseismic and Magnetic Imager on board Solar Dynamics Observatory) Active Region Patches (SHARPs), which are two currently avai…

2024 The Astrophysical Journal
SOHO 2
Time-resolved Hubble Space Telescope Wide Field Camera 3 Spectrophotometry Reveals Inefficient Day-to-night Heat Redistribution in the Highly Irradiated Brown Dwarf SDSS 1557B
DOI: 10.3847/1538-4357/ad354c Bibcode: 2024ApJ...966....4A

Mayorga, L. C.; Lothringer, Joshua D.; Apai, Dániel +8 more

Brown dwarfs (BDs) in ultra-short-period orbits around white dwarfs (WDs) offer a unique opportunity to study the properties of tidally locked, fast-rotating (1–3 hr), and highly irradiated atmospheres. Here we present phase-resolved spectrophotometry of the WD–BD binary SDSS 1557, which is the fifth WD–BD binary in our six-object sample. Using th…

2024 The Astrophysical Journal
Gaia eHST 2
M 1-92: The Death of an AGB Star Told by Its Isotopic Ratios
DOI: 10.3390/galaxies12050063 Bibcode: 2024Galax..12...63M

Sánchez Contreras, Carmen; Masa, Elisa; Alcolea, Javier +3 more

Ongoing improvements in the sensitivity of sub-mm- and mm-range interferometers and single-dish radio telescopes allow for the increasingly detailed study of AGB and post-AGB objects in molecular species other than CO12

2024 Galaxies
Herschel 2
An Extremely Young Protostellar Core, MMS 1/OMC-3: Episodic Mass Ejection History Traced by the Micro SiO Jet
DOI: 10.3847/1538-4357/ad2268 Bibcode: 2024ApJ...964...48T

Herczeg, Gregory J.; Johnstone, Doug; Mairs, Steve +11 more

We present ∼0.″2 (∼80 au) resolution observations of the CO(2–1) and SiO(5–4) lines made with the Atacama large millimeter/submillimeter array toward an extremely young intermediate-mass protostellar source (t dyn < 1000 yr), MMS 1 located in the Orion Molecular Cloud-3 region. We have successfully imaged a very compact CO molecular …

2024 The Astrophysical Journal
Gaia 2