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The Blanco DECam Bulge Survey (BDBS). VIII. Chemo-kinematics in the southern Galactic bulge from 2.3 million red clump stars with Gaia DR3 proper motions
DOI: 10.1051/0004-6361/202347570 Bibcode: 2024A&A...682A..96M

Rich, R. Michael; Kunder, Andrea; Johnson, Christian I. +5 more

Context. The inner Galaxy is a complex environment, and the relative contributions of different formation scenarios to its observed morphology and stellar properties are still debated. The different components are expected to have different spatial, kinematic, and metallicity distributions, and a combination of photometric, spectroscopic, and astr…

2024 Astronomy and Astrophysics
Gaia 1
MeerKAT reveals a ghostly thermal radio ring towards the Galactic Centre
DOI: 10.1051/0004-6361/202450766 Bibcode: 2024A&A...690A..53B

Lundqvist, P.; Umana, G.; Filipović, M. D. +26 more

We present the serendipitous discovery of a new radio-continuum ring-like object nicknamed Kýklos (J1802–3353), with MeerKAT UHF and L-band observations. The radio ring, which resembles the recently discovered odd radio circles (ORCs), has a diameter of ∼80″ and is located just ∼6° from the Galactic plane. However, Kýklos exhibits an atypical ther…

2024 Astronomy and Astrophysics
Gaia 1
CME Arrival Time Prediction via Fusion of Physical Parameters and Image Features
DOI: 10.3847/1538-4365/ad1f5d Bibcode: 2024ApJS..271...31Z

Xu, Long; Huang, Xin; Zhao, Dong +1 more

Coronal mass ejections (CMEs) are among the most intense phenomena in the Sun–Earth system, often resulting in space environment effects and consequential geomagnetic disturbances. Consequently, quickly and accurately predicting CME arrival time is crucial to minimize the harm caused to the near-Earth space environment. To forecast the arrival tim…

2024 The Astrophysical Journal Supplement Series
SOHO 1
Mid-infrared Fine Structure Lines from the Galactic Warm Ionized Medium
DOI: 10.1088/1538-3873/ace6d9 Bibcode: 2024PASP..136e4301K

Kulkarni, S. R.; Beichman, Charles; Ressler, Michael E.

The Warm Ionized Medium (WIM) hosts most of the ionized gas in the Galaxy and occupies perhaps a quarter of the volume of the Galactic disk. Decoding the spectrum of the Galactic diffuse ionizing field is of fundamental interest. This can be done via direct measurements of ionization fractions of various elements. Based on current physical models …

2024 Publications of the Astronomical Society of the Pacific
JWST 1
The Spatial Correlation between CN-line- and Dust-continuum-emitting Regions in High-mass Star-forming Clouds
DOI: 10.3847/1538-4357/ad7019 Bibcode: 2024ApJ...974..231H

Hwang, Jihye; Chung, Eun Jung; Kim, Jongsoo +2 more

Measuring the strength of a three-dimensional (3D) magnetic field vector is challenging as it is not easy to recognize whether its line-of-sight (LOS) and plane-of-sky (POS) components are obtained from the same region. CN (N = 1–0) emission has been used to get the LOS component of a magnetic field (B LOS) from its Zeeman splitting lin…

2024 The Astrophysical Journal
Herschel 1
Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
DOI: 10.1051/0004-6361/202451324 Bibcode: 2024A&A...690A.347R

Hamann, W. -R.; Bozzo, E.; Soria, R. +11 more

Context. Ultra-luminous X-ray sources (ULXs) are high-mass X-ray binaries with an X-ray luminosity above 1039 erg s‑1. These ULXs can be powered by black holes that are more massive than 20 M, accreting in a standard regime, or lighter compact objects accreting supercritically. There are only a few ULXs with known…

2024 Astronomy and Astrophysics
XMM-Newton eHST 1
Accretion versus core-filament collision: Implications for streamer formation in Per-emb-2
DOI: 10.1051/0004-6361/202450854 Bibcode: 2024A&A...690L...3N

Nakamura, Fumitaka; Nguyen-Luong, Quang; Ishihara, Kousuke +1 more

Context. Recent millimetre and sub-millimetre observations have unveiled elongated and asymmetric structures around protostars. These structures, referred to as streamers, often exhibit coherent velocity gradients, seemingly indicating a directed gas flow towards the protostars. However, their origin and role in star formation remain uncertain. Ai…

2024 Astronomy and Astrophysics
Herschel 1
Characterization of the Blue Straggler Star Populations, through Statistical, Photometric, and Spectral Energy Distribution Analysis, in the Old Open Cluster: NGC 2243
DOI: 10.3847/1538-3881/ad84eb Bibcode: 2024AJ....168..274S

Medhi, Biman J.; Sheikh, A. H.

We present a statistical, photometric, and spectral energy distribution (SED) analysis of the poorly studied old open cluster: NGC 2243, to characterize its blue straggler star (BSS) population. We applied ensemble-based unsupervised machine learning methods to estimate the membership probabilities using Gaia Data Release 3 (DR3) astrometric data.…

2024 The Astronomical Journal
Gaia 1
A Multiwavelength Machine-learning Approach to Classifying X-Ray Sources in the Fields of Unidentified 4FGL-DR4 Sources
DOI: 10.3847/1538-4357/ad543e Bibcode: 2024ApJ...971..180Y

Kargaltsev, Oleg; Yang, Hui; Hare, Jeremy

A large fraction of Fermi-Large Area Telescope (LAT) sources in the fourth Fermi-LAT 14 yr catalog (4FGL) still remain unidentified (unIDed). We continued to improve our machine-learning pipeline and used it to classify 1206 X-ray sources with signal-to-noise ratios >3 located within the extent of 73 unIDed 4FGL sources with Chandra X-ray Obser…

2024 The Astrophysical Journal
Gaia 1
Diverse volcanism and crustal recycling on early Mars
DOI: 10.1038/s41550-023-02191-7 Bibcode: 2024NatAs...8..456M

Xiao, Long; Edwards, Christopher S.; Michalski, Joseph R. +2 more

The relatively well-preserved ancient crust of Mars provides a natural window into early planetary evolution not available on Earth due to sustained tectonic recycling and erosion on this planet. Mars has generally been considered a one-plate basaltic planet, though recent evidence suggests magmatic evolution resulting in felsic crust might have o…

2024 Nature Astronomy
MEx 1