Search Publications

Tracing the Propagation of Shocks in the Equatorial Ring of SN 1987A over Decades with the Hubble Space Telescope
DOI: 10.3847/1538-4357/ad812e Bibcode: 2024ApJ...976..164T

Fransson, Claes; Larsson, Josefin; Tegkelidis, Christos

The nearby SN 1987A offers a unique opportunity to investigate the complex shock interaction between the ejecta and circumstellar medium. We track the evolution of the optical hot spots within the equatorial ring (ER) by analyzing 33 Hubble Space Telescope imaging observations between 1994 and 2022. By fitting the ER with an elliptical model, we d…

2024 The Astrophysical Journal
eHST 0
X-Ray Emission of Nearby Low-mass and Sunlike Stars with Directly Imageable Habitable Zones
DOI: 10.3847/1538-4365/ad71d6 Bibcode: 2024ApJS..275....1B

Peacock, Sarah; Kane, Stephen R.; Schwieterman, Edward W. +5 more

Stellar X-ray and UV radiation can significantly affect the survival, composition, and long-term evolution of the atmospheres of planets in or near their host star's habitable zone (HZ). Especially interesting are planetary systems in the solar neighborhood that may host temperate and potentially habitable surface conditions, which may be analyzed…

2024 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 0
Classifying the clouds of Venus using unsupervised machine learning
DOI: 10.1016/j.ascom.2024.100884 Bibcode: 2024A&C....4900884M

Molaverdikhani, K.; Grassi, T.; Ercolano, B. +2 more

Because Venus is completely shrouded by clouds, they play an important role in the planet's atmospheric dynamics. Studying the various morphological features observed on satellite imagery of the Venusian clouds is crucial to understanding not only the dynamic atmospheric processes, but also interactions between the planet's surface structures and …

2024 Astronomy and Computing
VenusExpress 0
A Diamond Ring in X-Ray: Investigating the Diffuse Emission of Supernova Remnant G28.8+1.5
DOI: 10.1088/1538-3873/ad6105 Bibcode: 2024PASP..136g4301Z

Zhang, Kaiyue

Supernova remnants are products of supernova explosions, which are usually observed in the X-ray band. However, the diffuse emission from the galactic supernova remnant G28.8+1.5 has been overlooked following initial searches for pulsars and pulsar wind nebulae. This paper presents background-subtracted imaging and spatial-resolved spectral analys…

2024 Publications of the Astronomical Society of the Pacific
XMM-Newton 0
Millisecond pulsars phenomenology under the light of graph theory
DOI: 10.1051/0004-6361/202450758 Bibcode: 2024A&A...692A.187G

de Martino, D.; Torres, D. F.; Papitto, A. +4 more

We compute and apply the minimum spanning tree (MST) of the binary millisecond pulsar population, and discuss aspects of the known phenomenology of these systems in this context. We find that the MST effectively separates different classes of spider pulsars – eclipsing radio pulsars in tight binary systems with a companion of either ~0.1–0.8 M

2024 Astronomy and Astrophysics
XMM-Newton 0
Comparison of Direct Magnetic Field Measurements in a Sunspot by Ten Spectral Lines of Fe I, Fe II, Ti I, and Ti II
DOI: 10.3103/S0884591324060047 Bibcode: 2024KPCB...40..337L

Lozitsky, V. G.; Lozitska, N. I.; Yakovkin, I. I. +1 more

Direct magnetic field measurements in sunspots by many spectral lines are important for elucidating the true magnitude and structure of the magnetic field at different levels of the solar atmosphere. Currently, magnetographic measurements are the most widespread, but such measurements mainly represent the longitudinal component of the magnetic fie…

2024 Kinematics and Physics of Celestial Bodies
SOHO 0
Compact ellipticals in the Antlia cluster of galaxies
DOI: 10.1051/0004-6361/202452113 Bibcode: 2024A&A...691A.307C

Richtler, Tom; Caso, Juan Pablo; Bassino, Lilia P. +3 more

Context. Compact ellipticals (cEs) are rare objects in the local Universe, but relevant for the evolution of galaxies. Their origin is not completely understood, with evidence equally suggesting that they are relics of early epochs, and remnants of tidal disruptions. Aims. This article aims to characterise two cEs, members of the nearby Antlia clu…

2024 Astronomy and Astrophysics
eHST 0
Ultra-Low Frequency Waves of Foreshock Origin Upstream and Inside of the Magnetospheres of Earth, Mercury, and Saturn Related to Solar Wind–Magnetosphere Coupling
DOI: 10.3390/universe10110407 Bibcode: 2024Univ...10..407B

Juhász, Antal; Bebesi, Zsofia; Dwivedi, Navin Kumar +2 more

This review examines ultra-low frequency (ULF) waves across different planetary environments, focusing on Earth, Mercury, and Saturn. Data from spacecraft missions (CHAMP, Swarm, and Oersted for Earth; MESSENGER for Mercury; and Cassini for Saturn) provide insights into ULF wave dynamics. At Earth, compressional ULF waves, particularly Pc3 waves, …

2024 Universe
Cluster 0
Witt's Hyperbola Is Both Predicted and Observed to Pass Close to the Lensing Galaxies in Quadruple Quasars
DOI: 10.3847/1538-4357/ad7f4d Bibcode: 2024ApJ...975...62S

Schechter, Paul L.; Luhtaru, Richard

When a rectangular hyperbola is constructed from the image positions of a quadruply lensed quasar, as proposed by Witt, it passes very close to the lensing galaxy. The median measured perpendicular offset between the observed light center of the lens and Witt's hyperbola is 0.″013 for a sample for 39 systems lensed by a relatively isolated galaxy.…

2024 The Astrophysical Journal
Gaia eHST 0
ASASSN-21js: A multi-year transit of a ringed disc
DOI: 10.1051/0004-6361/202450288 Bibcode: 2024A&A...688L..11P

van Boekel, R.; Kenworthy, M. A.; Pramono, T. H.


Aims: The early-type star ASASSN-21js started to fade in 2021, as was detected by the All Sky Automated Survey for Supernovae, undergoing a multi-year eclipse that is still underway. We interpret this event as being due to a structured disc of material transiting in front of the star. The disc is in orbit around a substellar object with the m…

2024 Astronomy and Astrophysics
Gaia 0