Search Publications

The existence of hot X-ray onsets in solar flares
DOI: 10.1051/0004-6361/202347706 Bibcode: 2023A&A...679A.139B

Krucker, Säm; Veronig, Astrid M.; Dickson, Ewan C. M. +9 more

Context. It is well known among the scientific community that solar flare activity often begins well before the main impulsive energy release. However, a consistent explanation for this phenomenon has not yet been established.
Aims: Our aim is to investigate the earliest phase of four distinct flares observed by Solar Orbiter/STIX and determi…

2023 Astronomy and Astrophysics
SolarOrbiter 8
Multi-campaign asteroseismic analysis of eight solar-like pulsating stars observed by the K2 mission
DOI: 10.1051/0004-6361/202244577 Bibcode: 2023A&A...674A.106G

García, R. A.; Pérez Hernández, F.; Mathur, S. +11 more

The NASA K2 mission that succeeded the nominal Kepler mission observed several hundred thousand stars during its operations. While most of the stars were observed in single campaigns of ∼80 days, some of them were targeted for more than one campaign. We perform an asteroseismic study of a sample of eight solar-like stars observed during K2 Campaig…

2023 Astronomy and Astrophysics
Gaia 8
Far-ultraviolet Spectroscopy of Active Galactic Nuclei with ASTROSAT/UVIT
DOI: 10.3847/1538-4357/acc941 Bibcode: 2023ApJ...950...90K

Papadakis, I. E.; Singh, K. P.; Dewangan, G. C. +4 more

We study accretion disk emission from eight Seyfert 1-1.5 active galactic nuclei (AGN) using far-ultraviolet (FUV) (1300-1800 Å) slitless grating spectra acquired with AstroSat/UVIT. We correct for the Galactic and intrinsic extinction, contamination from the host galaxies, narrow and broad-line regions, Fe II emission, and Balmer continuum, and d…

2023 The Astrophysical Journal
eHST 8
Hazy with a Chance of Star Spots: Constraining the Atmosphere of Young Planet K2-33b
DOI: 10.3847/1538-3881/aca07a Bibcode: 2023AJ....165...23T

Vanderburg, Andrew; Mann, Andrew W.; Irwin, Jonathan M. +10 more

Although all-sky surveys have led to the discovery of dozens of young planets, little is known about their atmospheres. Here, we present multiwavelength transit data for the super-Neptune sized exoplanet, K2-33b-the youngest (~10 Myr) transiting exoplanet to date. We combined photometric observations of K2-33 covering a total of 33 transits spanni…

2023 The Astronomical Journal
eHST 8
Spectroscopic Orbits of Subsystems in Multiple Stars. X (Summary)
DOI: 10.3847/1538-3881/acca19 Bibcode: 2023AJ....165..220T

Tokovinin, Andrei

Results of a large program of spectroscopic monitoring of nearby solar-type stellar hierarchical systems using the CHIRON echelle spectrograph at the 1.5 m telescope are summarized. Ten papers of this series contain 102 spectroscopic orbits and substantially contribute to the knowledge of periods and eccentricties, providing input for the study of…

2023 The Astronomical Journal
Gaia 8
Tilted discs in six poorly studied cataclysmic variables
DOI: 10.1093/mnras/stad259 Bibcode: 2023MNRAS.520.3355S

Stefanov, Stefan Y.; Stefanov, Atanas K.

In this work, we search for negative superhumps (nSHs) in poorly studied cataclysmic variables using Transiting Exoplanet Survey Satellite data. We find three eclipsing binaries with nSH signatures: HBHA 4204-09, Gaia DR3 5931071148325476992, and SDSS J090113.51+144704.6. The last one exhibits IW And-like behaviour in archival Zwicky Transient Fac…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 8
On the General Correlation between 3D Solar Wind Speed and Density Model and Solar Proxies
DOI: 10.3847/1538-4365/ac9fd4 Bibcode: 2023ApJS..264...11P

Bzowski, M.; Tokumaru, M.; Porowski, C.

The solar wind (SW) is a supersonic outflow of plasma from the solar corona, with the latitudinal speed and density profiles varying with the solar activity. The SW protons charge exchange with the inflowing interstellar neutral atoms and create energetic neutral atoms (ENAs), which bring information on the physical state of the plasma within the …

2023 The Astrophysical Journal Supplement Series
Ulysses 8
Unraveling the Complex Structure of AGN-driven Outflows. VI. Strong Ionized Outflows in Type 1 AGNs and the Outflow Size-Luminosity Relation
DOI: 10.3847/1538-4357/acf92b Bibcode: 2023ApJ...958..145K

Luo, Rongxin; Chung, Aeree; Baek, Junhyun +4 more

We present spatially resolved gas kinematics, ionization, and energetics of 11 type 1 and 5 type 2 active galactic nuclei (AGNs) with strong ionized gas outflows at z <0.3 using Gemini Multi-Object Spectrograph Integral Field Unit data. We find a strongly blueshifted region in [O III] velocity maps, representing an approaching cone in biconical…

2023 The Astrophysical Journal
AKARI 8
Occurrence rate of hot Jupiters orbiting red giant stars
DOI: 10.1051/0004-6361/202244180 Bibcode: 2023A&A...670A..26T

Snellen, Ignas A. G.; Temmink, Milou

Context. Hot Jupiters form an enigmatic class of object whose formation pathways are not yet clear. Determining their occurrence rates as a function of orbit, planet and stellar mass, and system age can be an important ingredient for understanding how they form. To date, various hot Jupiters have been discovered orbiting red giant stars, and deriv…

2023 Astronomy and Astrophysics
Gaia 8
Solar Electron Beam-Langmuir Wave Interactions and How They Modify Solar Electron Beam Spectra: Solar Orbiter Observations of a Match Made in the Heliosphere
DOI: 10.3847/1538-4357/ad0be3 Bibcode: 2023ApJ...959..128L

Verscharen, Daniel; Maksimovic, Milan; Ryan, Daniel F. +7 more

Solar Orbiter's four in situ instruments have recorded numerous energetic electron events at heliocentric distances between 0.5 and 1 au. We analyze energetic electron fluxes, spectra, pitch-angle distributions, associated Langmuir waves, and type III solar radio bursts for three events to understand what causes modifications in the electron flux …

2023 The Astrophysical Journal
SolarOrbiter 8