Search Publications

Investigation of the nature of the wind interaction in HD 93205 based on multi-epoch X-ray observations
DOI: 10.1051/0004-6361/202451681 Bibcode: 2024A&A...692A..36A

De Becker, Michaël; Arora, Bharti

Context. The study of the X-ray emission from massive binaries constitutes a relevant approach to investigate shock physics. The case of short period binaries may turn out to be quite challenging, especially in very asymmetric systems where the primary wind may overwhelm that of the secondary in the wind interaction. Aims. Our objective consists i…

2024 Astronomy and Astrophysics
XMM-Newton 0
Fifty Years After the Discovery of the First Stellar-Mass Black Hole: A Review of Cyg X-1
DOI: 10.3390/galaxies12060080 Bibcode: 2024Galax..12...80J

Jiang, Jiachen

Around 50 years ago, the famous bet between Stephen Hawking and Kip Thorne on whether Cyg X-1 hosts a stellar-mass black hole became a well-known story in the history of black hole science. Today, Cyg X-1 is widely recognised as hosting a stellar-mass black hole with a mass of approximately 20 solar masses. With the advancement of X-ray telescopes…

2024 Galaxies
INTEGRAL 0
Multi-wavelength photometric study of five contact binaries in the field of globular cluster M4
DOI: 10.1016/j.newast.2023.102150 Bibcode: 2024NewA..10702150D

Brosch, Noah; Jagirdar, Rukmini; Devarapalli, Shanti Priya +4 more

Binary stars are believed to be key determinants in understanding globular cluster evolution. In this paper, we present the Multi-band photometric analyses of five variables in the nearest galactic globular cluster M4, from the observations of CASE, M4 Core Project with HST for four variables (V48, V49, V51, and V55) and the data collected from T4…

2024 New Astronomy
eHST 0
Supernova Shocks in Molecular Clouds: Shocks Driven into Dense Cores in IC 443 and 3C 391
DOI: 10.3847/1538-4357/ad8d59 Bibcode: 2024ApJ...977..149R

Tram, Le Ngoc; Reach, William T.; Godard, Benjamin +3 more

Supernova shocks into dense molecular cores in IC 443 (clumps B, C, and G) and 3C 391 were observed using the Stratospheric Observatory for Infrared Astronomy and complemented by archival data from the Herschel Space Observatory. The pure rotational transitions 0–0 S(1) and S(5) of H2, and the ground-state 110–101

2024 The Astrophysical Journal
Herschel 0
MARSIS data as a new constraint for the orbit of Phobos
DOI: 10.1051/0004-6361/202348655 Bibcode: 2024A&A...686A.136D

Orosei, R.; Lainey, V.; Cicchetti, A. +3 more

Context. The orbit of Phobos is currently known with a 1σ precision of 300 m, mostly directed along its track. Most previous determinations were made with the help of the Super-Resolution Channel (SRC) channel of the HRSC camera on board Mars Express (MEX). The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) on board MEX crosse…

2024 Astronomy and Astrophysics
MEx 0
A Targeted Search for Variable Gravitationally Lensed Quasars
DOI: 10.3847/1538-4357/ad5dad Bibcode: 2024ApJ...973...24S

Schlegel, David J.; Huang, Xiaosheng; Palmese, Antonella +4 more

We present a pipeline to identify photometric variability within strong gravitationally lensing candidates, in the Dark Energy Spectroscopic Instrument Legacy Imaging Surveys. In our first paper, we laid out our pipeline and presented seven new gravitationally lensed supernovae candidates in a retrospective search. In this companion paper, we appl…

2024 The Astrophysical Journal
eHST 0
Chemical abundances in nearby Sun-like stars and the history of the Milky Way disc
DOI: 10.1051/0004-6361/202449820 Bibcode: 2024A&A...690A.369G

Gondoin, P.

Context. The properties of nearby stars bear the imprint of the formation and evolution of the Milky Way (MW). Reconstructing its history requires the determination of precise ages for large samples of stars over long periods. Aims. The present study aims to address the evolution of the MW disc in the region where the Sun and nearby Sun-like stars…

2024 Astronomy and Astrophysics
Gaia 0
Horizontal branch structure, age, and chemical composition for very metal-poor extragalactic globular clusters
DOI: 10.1093/mnras/stae426 Bibcode: 2024MNRAS.528.7165S

Sharina, M. E.; Kniazev, A. Y.; Shimansky, V. V. +2 more

This paper presents the results of analysing the integrated light (IL) low-resolution spectra of globular clusters (GCs) in the M31 and Centaurus A groups of galaxies. The sample consists of eight very metal-poor GCs ($\rm [Fe/H]\le -2$ dex) with high signal-to-noise ratio spectra acquired with the telescopes: the 6-m SAO RAS (BTA), the Southern A…

2024 Monthly Notices of the Royal Astronomical Society
eHST 0
A Spatial Uniformity Check of Gaia DR3 Photometry and BP/RP Spectra
DOI: 10.3847/1538-4357/ad70ab Bibcode: 2024ApJ...973....1H

Huang, Bowen; Yuan, Haibo; Xiao, Kai

Gaia DR3 photometry and Blue Photometer (BP) and Red Photometer (RP) spectra have been widely used as reference in photometric calibrations. In this work, we check the spatial uniformity of Gaia DR3 photometry and BP/RP spectra by comparing the BP, RP, and G-band photometry with the synthetic ones from the BP/RP spectra. The discrepancies have a s…

2024 The Astrophysical Journal
Gaia 0
Sigmoid Eruption Associated with the X9.3 Flare from AR 12673 Drives the Gradual Solar Energetic Particle Event on 2017 September 6
DOI: 10.3847/1538-4357/ad8d5f Bibcode: 2024ApJ...976..152Y

Brooks, David H.; Yardley, Stephanie L.

Large gradual solar energetic particle (SEP) events can pose a radiation risk to crewed spaceflight and a significant threat to near-Earth satellites; however, the origin of the SEP seed particle population, and how these particles are released, accelerated and transported into the heliosphere are not well understood. We analyze NOAA active region…

2024 The Astrophysical Journal
Hinode SOHO 0