Search Publications

Probing the emission mechanism and nature of the pulsating compact object in the X-ray binary SAX J1324.4−6200
DOI: 10.1051/0004-6361/202349033 Bibcode: 2024A&A...685A.148D

Santangelo, A.; Serim, M. M.; Ducci, L. +6 more

Recently, there has been renewed interest in the Be X-ray binary (Be/XRB) SAX J1324.4−6200 because of its spatial coincidence with a variable γ-ray source detected by Fermi/LAT. To explore more thoroughly its properties, new X-ray observations were carried out in 2023 by NuSTAR, XMM-Newton, and Swift satellites, jointly covering the energy range f…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 0
DECam Multimessenger Astrophysics Pipeline. I. From Raw Data to Single-exposure Candidates
DOI: 10.3847/1538-3881/ad70b1 Bibcode: 2024AJ....168..186F

Matheson, Thomas; Meisner, Aaron; Fu, Shenming +3 more

We introduce a pipeline that performs rapid image subtraction and source selection to detect transients, with a focus on identifying gravitational-wave optical counterparts using the Dark Energy Camera (DECam). In this work, we present the pipeline steps from processing raw data to identification of astrophysical transients on individual exposures…

2024 The Astronomical Journal
Gaia 0
The chemical evolution of the Milky Way thin disk using solar twins
DOI: 10.1051/0004-6361/202451167 Bibcode: 2024A&A...691A.298P

Spina, L.; Carraro, G.; Casali, G. +2 more

Aims. In this study we address whether the age-metallicity relation (AMR) deviates from the expected trend of metallicity increasing smoothly with age. We also show the presence (or absence) of two populations, as recently claimed using a relatively small dataset. Moreover, we studied the Milky Way thin disk's chemical evolution using solar twins,…

2024 Astronomy and Astrophysics
Gaia 0
Hot bubbles of planetary nebulae with hydrogen-deficient winds. III. Formation and evolution in comparison with hydrogen-rich bubbles
DOI: 10.1051/0004-6361/202346170 Bibcode: 2024A&A...684A.105S

Steffen, M.; Schönberner, D.


Aims: We seek to understand the evolution of Wolf-Rayet central stars by comparing the diffuse X-ray emission from their windblown bubbles with that from their hydrogen-rich counterparts with predictions from hydrodynamical models.
Methods: We simulate the dynamical evolution of heat-conducting wind-blown bubbles using our 1D radiation-h…

2024 Astronomy and Astrophysics
Gaia 0
Valley Relief of the Northeastern Part of Terra Cimmeria on Mars
DOI: 10.1134/S0038094624700175 Bibcode: 2024SoSyR..58..269M

Mukhamedzhanova, A. E.

A study of the valley topography of the northeastern part of Terra Cimmeria on Mars was carried out. The results of the study allow us to draw the following conclusions. (1) The morphology of the studied valley systems corresponds to their presumed fluvial origin. (2) The remains of the paleodelta in the Gusev crater, fragments of terrace levels t…

2024 Solar System Research
MEx 0
Search for the wide-orbit massive companion of XO-7b in the follow-up radial-velocity and transit-timing data: no significant clues
DOI: 10.1093/mnras/stad3418 Bibcode: 2024MNRAS.527.3474G

Garai, Z.; Pribulla, T.; Komžík, R.

XO-7b is a hot Jupiter transiting a V = 10.52 mag G0V-type star. The planetary system is interesting because the linear slope in the discovery radial-velocity (RV) data indicated a wide-orbit massive companion. In 2020 we started an RV campaign for the system with the main scientific goal to follow-up this linear slope, and to put constraints on t…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0
Investigation of WZ Sge-type Dwarf Nova ASASSN-19oc: Optical Spectroscopy and Multicolor Light Curve Analysis
DOI: 10.1088/1674-4527/ad59ec Bibcode: 2024RAA....24h5002K

Krushevska, Viktoriia; Shugarov, Sergey; Ochner, Paolo +3 more

In this study, we present an investigation of the newly discovered dwarf nova ASASSN-19oc during its superoutburst on 2019 June 2. We carried out detailed UBVR c I c -photometric observations and also obtained a spectrum on day 7 of the outburst, which shows the presence of hydrogen absorption lines commonly found in dwarf…

2024 Research in Astronomy and Astrophysics
Gaia 0
Origin of Line Broadening in Fading Granules: Influence of Small-scale Turbulence
DOI: 10.3847/1538-4357/ad71cd Bibcode: 2024ApJ...975...98I

Katsukawa, Yukio; Ishikawa, Ryohtaroh T.

In the quiet region of the solar photosphere, turbulent convective motions of the granular flows naturally drive the subgranular-scale flows. However, evaluating such small-scale velocities is challenging because of the limited instrumental resolution. Our previous study, R. T. Ishikawa et al., found line-broadening events during the fading proces…

2024 The Astrophysical Journal
Hinode 0
Gaia Data Release 3: Distribution of Spectral Groups of Near-Earth Asteroids
DOI: 10.1134/S0038094624700205 Bibcode: 2024SoSyR..58..359S

Kovaleva, D. A.; Shcherbina, M. P.; Shustov, B. M.

Based on the data from the third edition of the Gaia catalog, containing the reflectance spectra of asteroids, studies of near-Earth asteroids (NEAs) were carried out. The reflectance spectra of about 100 representatives of the Aten, Apollo and Amor groups were used to determine their spectral class. For 47 asteroids such an assessment was made fo…

2024 Solar System Research
Gaia 0
The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
DOI: 10.1051/0004-6361/202347826 Bibcode: 2024A&A...684A..31G

Krongold, Yair; Gallego, Jesús; Sánchez-Portal, Miguel +21 more

Context. The Lockman-SpReSO project is an optical spectroscopic survey of 956 far-infrared (FIR) objects within the Lockman Hole field limited by magnitude RC(AB) < 24.5. Fe II and Mg II absorption lines have been detected in 21 out of 456 objects with a determined spectroscopic redshift in the catalogue. The redshifts of these objec…

2024 Astronomy and Astrophysics
eHST 0