Search Publications

Solar Orbiter Observations of Proton and Alpha Particle Kinetic Signatures Related to the Presence of Switchbacks in the Inner Heliosphere: A Case Study
DOI: 10.3847/1538-4357/ad65db Bibcode: 2024ApJ...973..171P

Telloni, Daniele; D'Amicis, Raffaella; Perrone, Denise +6 more

We investigate how ions, namely protons and alpha particles, kinetically react to the presence of strong deflections in the magnetic field, the so-called switchbacks, in the first stream of slow Alfvénic wind observed by Solar Orbiter at the heliocentric distance of 0.64 au. We focus on an isolated, large-scale switchback, and we study in detail i…

2024 The Astrophysical Journal
SolarOrbiter 0
Source Region and Launch Characteristics of Magnetic-arch-blowout Solar Coronal Mass Ejections Driven by Homologous Compact-flare Blowout Jets
DOI: 10.3847/1538-4357/ad4995 Bibcode: 2024ApJ...969...48P

Joshi, Bhuwan; Moore, Ronald L.; Sterling, Alphonse C. +1 more

We study the formation of four coronal mass ejections (CMEs) originating from homologous blowout jets. All of the blowout jets originated from NOAA Active Region (AR) 11515 on 2012 July 2, within a time interval of ≈14 hr. All of the CMEs were wide (angular widths ≈ 95°–150°), and propagated with speeds ranging between ≈300 and 500 km s‑1

2024 The Astrophysical Journal
Hinode SOHO 0
Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System
DOI: 10.3847/1538-3881/ad2461 Bibcode: 2024AJ....167..155L

Butler, R. Paul; Kane, Stephen R.; Wittenmyer, Robert A. +16 more

Multiplanet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long observational baselines allow for searches for more distant planetary orbits. This work provides a significantly…

2024 The Astronomical Journal
Gaia 0
Nuclear structure and direct reaction studies in particle- γ coincidence experiments at the FSU John D. Fox superconducting linear accelerator laboratory
DOI: 10.3389/fphy.2024.1511394 Bibcode: 2024FrP....1211394S

Spieker, Mark-Christoph; Almaraz-Calderon, Sergio

Since its foundation in the 1960s, the John D. Fox Superconducting Linear Accelerator Laboratory at Florida State University (FSU) pursued research at the forefront of nuclear science. In this contribution, we present recent highlights from nuclear structure and reaction studies conducted at the John D. Fox Superconducting Linear Accelerator Labor…

2024 Frontiers in Physics
INTEGRAL 0
New orbital periods of high-inclination dwarf novae based on Gaia Alerts photometry
DOI: 10.1051/0004-6361/202451661 Bibcode: 2024A&A...691A.249S

Vogt, N.; Zorotovic, M.; Vega-Manubens, I. +8 more

The orbital period of a cataclysmic variable stands as a crucial parameter for investigating the structure and physics of these binary systems, as well as understanding their evolution. We use photometric Gaia data for dwarf novae (DNe) in the quiescent state – which are available for a number of years – to determine new orbital periods and improv…

2024 Astronomy and Astrophysics
Gaia 0
Long- and short-term variability of the possible nascent planetary nebula IRAS 22568+6141: A late thermal pulse?
DOI: 10.1051/0004-6361/202451719 Bibcode: 2024A&A...691A.321C

Miranda, Luis F.; Morisset, Christophe; Cala, Roldán A. +4 more

IRAS 22568+6141 has been classified as a low-excitation planetary nebula (PN) and presents non-thermal radio continuum emission, which could be a signature of a nascent PNe. We present intermediate-resolution long-slit spectra obtained in 2021 and 2023, high-resolution long-slit spectra taken in 2023, and a light curve at the r filter between 1953…

2024 Astronomy and Astrophysics
AKARI eHST 0
Investigation into the origin of the soft excess in Ark 564 using principal component analysis
DOI: 10.1051/0004-6361/202348783 Bibcode: 2024A&A...689A.116L

Yang, X. J.; Zhang, G. B.; Lyu, M. +1 more

We combined a principal component analysis (PCA) and spectroscopy to investigate the origin of the soft excess in narrow-line Seyfert 1 galaxy Ark 564 with XMM-Newton observations over a period of ten years. We find that the principal components in different epochs are very similar, suggesting stable variability patterns in this source. More impor…

2024 Astronomy and Astrophysics
XMM-Newton 0
Forgotten treasures in the HST/FOC UV imaging polarimetric archives of active galactic nuclei: III. Five years monitoring of M87
DOI: 10.1051/0004-6361/202451390 Bibcode: 2024A&A...692A.179M

Lopez-Rodriguez, E.; Marin, F.; Wu, K. +1 more

Context. The active galactic nucleus within M87, a giant elliptical galaxy, is responsible for one of the closest kiloparsec-scale relativistic jets to Earth. It is thus a perfect target for spatially resolved observations. Aims. This one-sided jet has been extensively observed at almost all wavelengths, with almost all techniques. Among many othe…

2024 Astronomy and Astrophysics
eHST 0
SMC-Last Extracted Photometry
DOI: 10.3847/1538-3881/ad2601 Bibcode: 2024AJ....167..149K

Boyer, M. L.; Oliveira, Joana M.; van Loon, Jacco Th. +11 more

We present point-source photometry from the Spitzer Space Telescope's final survey of the Small Magellanic Cloud (SMC). We mapped nearly 30 deg2 in two epochs in 2017, with the second extending to early 2018 at 3.6 and 4.5 µm using the Infrared Array Camera. This survey duplicates the footprint from the SAGE-SMC program in 2008. T…

2024 The Astronomical Journal
Gaia 0
Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique
DOI: 10.1051/0004-6361/202450033 Bibcode: 2024A&A...692A.149R

Hamann, W. -R.; Prinja, R. K.; Oskinova, L. M. +8 more

Context. NGC 346 is a young cluster with numerous hot OB stars. It is part of the Small Magellanic Cloud (SMC), and has an average metallicity that is one-seventh of the Milky Way's. A detailed study of its stellar content provides a unique opportunity to understand the stellar and wind properties of massive stars in low-metallicity environments, …

2024 Astronomy and Astrophysics
eHST 0