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The Black Hole Candidate Swift J1728.9-3613 and the Supernova Remnant G351.9-0.9
DOI: 10.3847/1538-4357/acc1c9 Bibcode: 2023ApJ...947...38B

Raymond, John; Ray, Paul S.; Zoghbi, Abderahmen +12 more

A number of neutron stars have been observed within the remnants of the core-collapse supernova explosions that created them. In contrast, black holes are not yet clearly associated with supernova remnants (SNRs). Indeed, some observations suggest that black holes are "born in the dark," i.e., without a supernova explosion. Herein, we present a mu…

2023 The Astrophysical Journal
XMM-Newton 4
AutoSourceID-FeatureExtractor. Optical image analysis using a two-step mean variance estimation network for feature estimation and uncertainty characterisation
DOI: 10.1051/0004-6361/202346983 Bibcode: 2023A&A...680A.108S

Groot, P. J.; Vreeswijk, P.; Nelemans, G. +9 more


Aims: In astronomy, machine learning has been successful in various tasks such as source localisation, classification, anomaly detection, and segmentation. However, feature regression remains an area with room for improvement. We aim to design a network that can accurately estimate sources' features and their uncertainties from single-band im…

2023 Astronomy and Astrophysics
Gaia 4
A Catalog of New Slowly Pulsating B-type Stars
DOI: 10.3847/1538-4365/ace88c Bibcode: 2023ApJS..268...16S

Shi, Xiang-dong; Qian, Sheng-bang; Zhu, Li-ying +1 more

This paper reports the discovery of new slowly pulsating B-type stars. Based on the photometric, spectral, and astrometric data of the TESS, LAMOST, and Gaia surveys, we have found 286 new slowly pulsating B-type (SPB) stars and 21 candidates. Among these, 20 are Be stars or candidates with emission-line profiles. It is shown that these SPB stars …

2023 The Astrophysical Journal Supplement Series
Gaia 4
X-ray emission from Ae/Be Herbig stars due to disc-stellar magnetosphere interaction
DOI: 10.1093/mnras/stad629 Bibcode: 2023MNRAS.521.2427R

Lyutikov, Maxim; Ryspaeva, Elizaveta; Kholtygin, Alexander

We reanalyse archival X-ray data of 16 Ae/Be Herbig stars obtained by the XMM-Newton and Chandra satellites. Stellar X-ray spectra in the energy range 0.2-8 keV were fitted with the use of APEC and MEKAL hot plasma emission models, and with models with an additional power-law component. We find that for Herbig stars, the dependence of the unabsorb…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 4
Multiple Rings and Asymmetric Structures in the Disk of SR 21
DOI: 10.3847/1538-4357/acc325 Bibcode: 2023ApJ...948..110Y

Dong, Ruobing; Tamura, Motohide; Liu, Hauyu Baobab +9 more

Crescent-like asymmetric dust structures discovered in protoplanetary disks indicate dust aggregations. Thus, researching these structures helps us understand the planet formation process. Here we analyze ALMA data of the protoplanetary disk around the T-Tauri star SR 21, which has asymmetric structures that were detected in previous submillimeter…

2023 The Astrophysical Journal
Gaia 4
NAROO program. Precovery observations of potentially hazardous asteroids
DOI: 10.1051/0004-6361/202347100 Bibcode: 2023A&A...680A..41P

Hestroffer, D.; Desmars, J.; Robert, V. +1 more

Context. The New Astrometric Reduction of Old Observations (NAROO) program is dedicated to the measurement of astrophotographic plates and the analysis of old observations for scientific purposes. One of the objectives of the NAROO program is to provide accurate positional measurements of small Solar System bodies in order to improve our knowledge…

2023 Astronomy and Astrophysics
Gaia 4
Field blue straggler stars: discovery of white dwarf companions to blue metal-poor stars using UVIT/AstroSat
DOI: 10.1093/mnras/stad2385 Bibcode: 2023MNRAS.525.1311P

Subramaniam, Annapurni; Panthi, Anju; Vaidya, Kaushar +4 more

Blue metal-poor (BMP) stars are the main-sequence stars that appear bluer and more luminous than normal turn-off stars of metal-poor globular clusters. They are believed to be either field blue straggler stars (FBSS) formed via post-mass transfer mechanism or accreted from dwarf satellite galaxies of the Milky Way. A significant fraction of BMP st…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
Everything that glitters is not gold: V1315 Cas is not a dormant black hole
DOI: 10.1093/mnras/stad2137 Bibcode: 2023MNRAS.524.5749Z

Guenther, E. W.; Shenar, T.; Boffin, H. M. J. +11 more

The quest for quiet or dormant black holes has been ongoing since several decades. Ellipsoidal variables possibly indicate the existence of a very high-mass invisible companion and are thought to be one of the best ways to find such dormant black holes. This, however, is not a panacea as we show here with one example. We indeed report the discover…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster
DOI: 10.3847/1538-4357/acc025 Bibcode: 2023ApJ...948...65L

Feldmeier-Krause, A.; Freedman, W. L.; Lonoce, Ilaria

The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local validity of general scaling relations. In this work, we present a direct comparison employing full spectral fittin…

2023 The Astrophysical Journal
eHST 4
Planar Magnetic Structures Downstream of Coronal Mass Ejection-driven Shocks in the Inner Heliosphere
DOI: 10.3847/1538-4357/acd245 Bibcode: 2023ApJ...951...47R

Xu, Qi; Feng, Xueshang; Shen, Zhenning +7 more

Planar magnetic structures (PMSs), characterized by interplanetary magnetic field vectors remaining parallel to a specific plane, are commonly observed in the solar wind, especially in the sheath region of interplanetary coronal mass ejections (ICMEs). In this study, PMS events in the 2 hr regions downstream of ICME-driven shocks were investigated…

2023 The Astrophysical Journal
SolarOrbiter VenusExpress 4