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Temporally Resolved Type III Solar Radio Bursts in the Frequency Range 3–13 MHz
DOI: 10.3847/2041-8213/ad7bbb Bibcode: 2024ApJ...974L..18V

Maksimovic, Milan; Kontar, Eduard P.; Chrysaphi, Nicolina +2 more

Radio observations from space allow to characterize solar radio bursts below the ionospheric cutoff, which are otherwise inaccessible, but suffer from low, insufficient temporal resolution. In this Letter we present novel, high-temporal resolution observations of type III solar radio bursts in the range 3–13 MHz. A dedicated configuration of the R…

2024 The Astrophysical Journal
SolarOrbiter 1
The MDW Hα Sky Survey: Data Release 0
DOI: 10.3847/1538-3881/ad7c48 Bibcode: 2024AJ....168..260A

Walker, Gary; Sliski, David H.; Schiminovich, David +9 more

The Mittelman–di Cicco–Walker (MDW) Hα Sky Survey is an autonomously operated and ongoing all-sky imaging survey in the narrowband Hα wavelength. The survey was founded by amateur astronomers and is presented here in its first stage of refinement for rigorous scientific use. Each field is exposed through an Hα filter with a 3 nm bandwidth for a to…

2024 The Astronomical Journal
Gaia 1
Investigating 56 High Galactic Latitude Open Cluster Candidates in Gaia DR3
DOI: 10.3847/1538-4357/ad2fbf Bibcode: 2024ApJ...965..131W

Chen, Jing; Zhang, Su; Wu, You +4 more

Using Gaia DR3 data, we revisit 56 high Galactic latitude (∣b∣ ≥ 30°) open cluster (OC) candidates with poor shapes of color–magnitude diagrams (CMDs), including unclear and paired main sequences (MSs). We aim to confirm their physical reality and explore whether the special MS morphology is intrinsic to genuine OCs. Initially, we redetermine clus…

2024 The Astrophysical Journal
Gaia 1
The Detection and Investigation of Exoplanets with MASTER Global Network Telescopes
DOI: 10.1134/S1063772924700513 Bibcode: 2024ARep...68..557L

Buckley, D. A. H.; Lipunov, V. M.; Budnev, N. M. +13 more

The paper presents the method for detecting exoplanets in the image archive obtained by telescopes of the MASTER Global Network since 2002. The unique archive represents homogeneous photometric data obtained over 20 years for the northern (MASTER-Amur, MASTER-Tunka, MASTER-Kislovodsk, M-ASTER-Tavrida, MASTER-IAC, MASTER-OAGH) and 11 years for the …

2024 Astronomy Reports
Gaia 1
Fundamental effective temperature measurements for eclipsing binary stars - V. The circumbinary planet system EBLM J0608-59
DOI: 10.1093/mnras/stae1434 Bibcode: 2024MNRAS.531.4577M

Maxted, P. F. L.; Martin, D. V.; Triaud, A. H. M. J. +3 more

EBLM J0608$-$59/TOI-1338/BEBOP-1 is a 12$^{\rm th}$-magnitude, F9 V star in an eclipsing binary with a much fainter M dwarf companion on a wide, eccentric orbit (P = 14.6 d). The binary is orbited by two circumbinary planets: one transiting on a 95-d orbit and one non-transiting on a 215-d orbit. We have used high-precision photometry from the TES…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
PSR J1227‑6208 and its massive white dwarf companion: Pulsar emission analysis, timing update, and mass measurements
DOI: 10.1051/0004-6361/202450724 Bibcode: 2024A&A...690A.253C

Freire, Paulo C. C.; Kramer, Michael; Champion, David J. +7 more

PSR J1227‑6208 is a 34.53-ms recycled pulsar with a massive companion. This system has long been suspected to belong to the emerging class of massive recycled pulsar‑ONeMg white dwarf systems such as PSR J2222‑0137, PSR J1528‑3146, and J1439‑5501. Here, we present an updated emission and timing analysis with more than 11 years of combined Parkes a…

2024 Astronomy and Astrophysics
Gaia 1
The Venus Global Ionosphere-Thermosphere Model (V-GITM): A Coupled Thermosphere and Ionosphere Formulation
DOI: 10.1029/2023JE008079 Bibcode: 2024JGRE..12908079P

Bougher, Stephen W.; Ridley, Aaron J.; Ponder, Brandon M. +2 more

This paper introduces the new Venus global ionosphere-thermosphere model (V-GITM) which incorporates the terrestrial GITM framework with Venus-specific parameters, ion-neutral chemistry, and radiative processes in order to simulate some of the observable features regarding the temperatures, composition, and dynamical structure of the Venus atmosph…

2024 Journal of Geophysical Research (Planets)
VenusExpress 1
Assessment of SDSS-derived Galaxy Morphologies Using HST Imaging
DOI: 10.3847/1538-4357/ad320f Bibcode: 2024ApJ...965..161O

Salim, Samir; Osborne, Chandler

The Sloan Digital Sky Survey (SDSS) was foundational to the study of galaxy evolution, having revealed the bimodality of galaxies and the relationship between their structure and star-forming activity. However, ground-based optical surveys like SDSS are limited in resolution and depth, which may lead to biases or poor quality in the derived morpho…

2024 The Astrophysical Journal
eHST 1
Massive Quiescent Disk Galaxies at 0.5 ≤ z ≤ 1 in CANDELS: Color Gradients and Likely Origin
DOI: 10.3847/1538-4357/ad6321 Bibcode: 2024ApJ...973...52C

Cui, Qifan; Liu, F. S.; Zhao, Pinsong

A rare population of massive disk-dominated quiescent galaxies has recently drawn much attention, which intrudes the red sequence (RS) population without destroying the underlying stellar disks. In this study, we have carefully identified 48 RS, disk-dominated galaxies with M * > 1010 M between redshift 0.5 an…

2024 The Astrophysical Journal
eHST 1
Period–Luminosity–Metallicity–Color Relations of Late-type Contact Binaries in the Big Data Era
DOI: 10.3847/1538-4357/ad12c0 Bibcode: 2024ApJ...961..248S

Tian, Zhi-Jia; Song, Lian-Yun

Binary stars ubiquitous throughout the Universe are important. Contact binaries (CBs) possessing period–luminosity (PL) relations could be adopted as distance tracers. The PL relations of CBs are influenced by metallicity abundance and color index, which are connected to both the radius and luminosity of stars. Here we propose fine relations of th…

2024 The Astrophysical Journal
Gaia 1