Search Publications

What drives the wheels of evolution in NGC 1512?. A UVIT study
DOI: 10.1051/0004-6361/202347412 Bibcode: 2024A&A...681A...7R

Mathew, Blesson; Kartha, Sreeja S.; George, Koshy +4 more

Context. Environmental and secular processes play a pivotal role in the evolution of galaxies. These can be external processes such as interactions or internal processes linked to the action of bar, bulge, and spiral structures. Ongoing star formation in spiral galaxies can be affected by these processes. By studying the star formation progression…

2024 Astronomy and Astrophysics
Gaia 2
Mapping and characterizing magnetic fields in the Rho Ophiuchus-A molecular cloud with SOFIA/HAWC+
DOI: 10.1051/0004-6361/202348008 Bibcode: 2024A&A...690A.191L

Diep, Pham Ngoc; Hoang, Thiem; Ngoc, Nguyen Bich +10 more

Context. Together with gravity, turbulence, and stellar feedback, magnetic fields (B-fields) are thought to play a critical role in the evolution of molecular clouds and star formation processes. The polarization of thermal dust emission is a popular tracer of B-fields in star-forming regions. Aims. We aim to map the morphology and measure the str…

2024 Astronomy and Astrophysics
Herschel 2
CME-Flare Association and the Role of Reconnection in CME Acceleration
DOI: 10.1007/s11207-024-02302-1 Bibcode: 2024SoPh..299...55R

Reva, Anton; Kirichenko, Alexey; Bogachev, Sergey +1 more

The association of coronal mass ejections (CMEs) with flares is related to the question of whether reconnection is necessary for the CME eruption. Indeed, if reconnection happens during a CME eruption, the plasma is heated, which can be observed as a flare. In this work, we study the CME-flare association using data obtained with the Mg XII spectr…

2024 Solar Physics
SOHO 2
Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78
DOI: 10.3847/2041-8213/ad5ffd Bibcode: 2024ApJ...970L..30X

Shi, Jianrong; Beers, Timothy C.; Allende Prieto, Carlos +9 more

Highly r-process-enhanced (RPE) stars are rare and usually metal poor ([Fe/H] < ‑1.0), and they mainly populate the Milky Way halo and dwarf galaxies. This study presents the discovery of a relatively bright (V = 12.72), highly RPE (r-II) star ([Eu/Fe] = +1.32, [Ba/Eu] = ‑0.95), LAMOST J020623.21+494127.9. This star was selected from the Large …

2024 The Astrophysical Journal
Gaia 2
Analysis of the Gaia Data Release 3 parallax bias in the Galactic plane
DOI: 10.1051/0004-6361/202450967 Bibcode: 2024A&A...691A..81D

Ding, Ye; Liao, Shilong; Qi, Zhaoxiang +2 more

Context. Systematic errors are inevitable in Gaia published astrometric data. A global recipe has been proposed to correct for the GEDR3 parallax zero-point offset, but this does not take the Galactic plane into consideration. The applicability of their correction model to the Galactic plane remains uncertain. Aims. We attempt to carry out an inde…

2024 Astronomy and Astrophysics
Gaia eHST 2
A clustering (DBSCAN+GMM) investigation of the young open cluster NGC 6649
DOI: 10.1093/mnras/stad3358 Bibcode: 2024MNRAS.527.1784G

Gao, Xinhua

We investigate the spatial structure and dynamical properties of the young (~60 Myr), richly populated open cluster NGC 6649 based on reliable cluster members from Gaia-DR3 data. The density-based spatial clustering of applications with noise is used to estimate membership probabilities for 25045 sample stars in the field of the cluster. More than…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Unveiling the origin of XMM-Newton soft proton flares: I. Design and validation of a response matrix for proton spectral analysis
DOI: 10.1051/0004-6361/202451231 Bibcode: 2024A&A...691A.229F

Cappi, M.; Molendi, S.; Gastaldello, F. +8 more

Context. Low-energy (<300 keV) protons entering the field of view of XMM-Newton can scatter with the X-ray mirror surface and reach the focal plane. They are observed in the form of a sudden increase in the background level, the so-called soft proton flares, affecting up to 40% of the mission observing time. Soft protons can hardly be disentang…

2024 Astronomy and Astrophysics
XMM-Newton 2
Detection of a new sample of Galactic white dwarfs in the direction of the Small Magellanic Cloud
DOI: 10.1051/0004-6361/202450292 Bibcode: 2024A&A...690A..68S

Arun, R.; Stalin, C. S.; Bhattacharyya, S. +7 more

Aims. In this study, we demonstrate the efficacy of the Ultraviolet Imaging Telescope (UVIT) in identifying and characterizing white dwarfs (WDs) within the Milky Way Galaxy. Methods. Leveraging the UVIT point-source catalogue towards the Small Magellanic Cloud and cross-matching it with Gaia DR3 data, we identified 43 single WDs (37 new detection…

2024 Astronomy and Astrophysics
Gaia 2
The Missing Symbiotic Stars: A Joint Analysis with Gaia, GALEX, and XMM-Newton Data
DOI: 10.3847/1538-4357/ad20ec Bibcode: 2024ApJ...962..126X

Shao, Yong; Li, Xiang-Dong; Xu, Xiao-jie

The existence of a population of low-accretion-rate symbiotic stars (SySts), consisting of a giant star and a compact companion (usually a white dwarf), has been proposed recently. However, their population has not been fully understood. In this work, we present an investigation on SySts candidates consisting of asymptotic giant branch stars (AGBs…

2024 The Astrophysical Journal
Gaia XMM-Newton 2
TIC 435850195: The Second Triaxial Tidally Tilted Pulsator
DOI: 10.3847/1538-4357/ad77c3 Bibcode: 2024ApJ...975..121J

Rappaport, Saul A.; Gagliano, Robert; Jayaraman, Rahul +8 more

The Transiting Exoplanet Survey Satellite (TESS) has enabled the discovery of numerous tidally tilted pulsators (TTPs), which are pulsating stars in close binaries where the presence of a tidal bulge has the effect of tilting the primary star's pulsation axes into the orbital plane. Recently, the modeling framework developed to analyze TTPs has be…

2024 The Astrophysical Journal
Gaia 2