Search Publications

The corona of a fully convective star with a near-polar flare
DOI: 10.1051/0004-6361/202449541 Bibcode: 2024A&A...687A.138I

Stelzer, B.; Poppenhäger, K.; Ilin, E. +1 more

Context. In 2020, the Transiting Exoplanet Survey Satellite (TESS) observed a rapidly rotating M7 dwarf, TIC 277539431, producing a flare at 81° latitude, the highest latitude flare located to date. This is in stark contrast to solar flares that occur much closer to the equator, typically below 30°. The mechanisms that allow flares at high latitud…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 0
Variation in the intensity ratio at each wavelength point of the Si IV 1394/1403 Å lines: Spectral diagnostics of a bifurcated eruption
DOI: 10.1051/0004-6361/202449488 Bibcode: 2024A&A...692A.210Z

Xu, Zhe; Xue, Zhike; Yan, Xiaoli +3 more

Aims. This study aims to investigate the deviation of the intensity ratio of the Si IV 1394 Å and 1403 Å emission lines from the expected value of 2 in the optically thin regime, as has been observed in many recent studies. Methods. We analyzed the integrated intensity ratio (R) and the wavelength-dependent ratio (r(Δλ)) in a small bifurcated erup…

2024 Astronomy and Astrophysics
IRIS 0
MOSEL survey: Unwrapping the Epoch of Reionisation through mimic galaxies at Cosmic Noon
DOI: 10.1017/pasa.2024.37 Bibcode: 2024PASA...41...40J

Harshan, Anishya; Gupta, Anshu; Trott, Cathryn M. +4 more

The nature of the first galaxies that reionised the universe during the Epoch of Reionisation (EoR) remains unclear. Attempts to directly determine spectral properties of these early galaxies are affected by both limited photometric constraints across the spectrum and by the opacity of the intergalactic medium to the Lyman Continuum (LyC) at high …

2024 Publications of the Astronomical Society of Australia
eHST JWST 0
Two Young Eclipsing Binaries in Orion with Temperatures and Radii Affected by Spots and Third Bodies
DOI: 10.3847/1538-3881/ad6a17 Bibcode: 2024AJ....168..134K

Stassun, Keivan G.; Kounkel, Marina

In this work we present a model of two young eclipsing binaries in the Orion complex. Both heavily spotted, they present radii and temperatures that are in disagreement with the predictions of standard stellar models. 2M05‑06 consists of two stars with different masses (∼0.52 and ∼0.42 M ) but with very similar radii (∼0.9 R

2024 The Astronomical Journal
Gaia 0
Analysis of faults and pit chains in Noctis Labyrinthus: Implications for early extension and possible magmatic plumbing
DOI: 10.1016/j.icarus.2024.116075 Bibcode: 2024Icar..41516075E

Sefton-Nash, Elliot; De Marchi, Guido; D'Incecco, Piero +10 more

Noctis Labyrinthus has been a region of disputed origin due to its complexity and poor understanding of how various processes and mechanisms may have combined to form it. The surface is an integrated record of intensive tectonic activity expressed by a multiple extended sets of dip-slip faults oriented in different directions, and thought to have …

2024 Icarus
MEx 0
The deep eclipses of RW Aur revisited by long-term photometric and spectroscopic monitoring
DOI: 10.1002/asna.20230118 Bibcode: 2024AN....34530118L

Mugrauer, Markus; Lux, Oliver; Bischoff, Richard

RW Aurigae is a young stellar system containing a classical T Tauri star as the primary component. It shows deep, irregular dimmings, first detected in 2010. At the University Observatory Jena, we carried out optical follow-up observations. We performed multiband (BVRI) photometry of the system with the Cassegrain-Teleskop-Kamera II and the Schmid…

2024 Astronomische Nachrichten
Gaia 0
HX Velorum: Ellipsoidal/Rotational Binary With β Cep Type Component
DOI: 10.1002/asna.20240028 Bibcode: 2024AN....34540028G

Gürol, B.

We present the Transiting Exoplanet Survey Satellite (TESS) light curve analysis of HX Velorum, located in the Southern Hemisphere, where one of the components is found for the first time to be a β$$ \beta $$ Cep (BCEP) type pulsator. The TESS observations of HX Velorum were published in a total of 6 sectors. Fourier analysis of the observations r…

2024 Astronomische Nachrichten
Gaia 0
The TESS–Keck Survey. XIX. A Warm Transiting Sub-Saturn-mass Planet and a Nontransiting Saturn-mass Planet Orbiting a Solar Analog
DOI: 10.3847/1538-3881/ad2765 Bibcode: 2024AJ....167..151H

Batalha, Natalie M.; Bieryla, Allyson; Latham, David W. +45 more

The Transiting Exoplanet Survey Satellite (TESS) continues to increase dramatically the number of known transiting exoplanets, and is optimal for monitoring bright stars amenable to radial velocity (RV) and atmospheric follow-up observations. TOI-1386 is a solar-type (G5V) star that was detected via TESS photometry to exhibit transit signatures in…

2024 The Astronomical Journal
Gaia 0
New Anisotropic Cosmic-Ray Enhancement (ACRE) Event on 5 November 2023 Due to Complex Heliospheric Conditions
DOI: 10.1007/s11207-024-02338-3 Bibcode: 2024SoPh..299...97G

Larsen, Nicholas; Gil, Agnieszka; Usoskin, Ilya +2 more

The variability of galactic cosmic rays near Earth is nearly isotropic and driven by large-scale heliospheric modulation but rarely can very local anisotropic events be observed in low-energy cosmic rays. These anisotropic cosmic-ray enhancement (ACRE) events are related to interplanetary transients. Until now, two such events have been known. Her…

2024 Solar Physics
SOHO 0
Herschel investigation of cores and filamentary structures in L1251 located in the Cepheus flare
DOI: 10.1007/s12036-024-10004-0 Bibcode: 2024JApA...45...19D

Soam, Archana; Zhang, Guo-Yin; Dewan, Divyansh +3 more

Molecular clouds are the prime locations of star formation. These clouds contain filamentary structures and cores which are crucial in the formation of young stars. In this work, we aim to quantify the physical properties of structural characteristics within the molecular cloud L1251 to better understand the initial conditions for star formation. …

2024 Journal of Astrophysics and Astronomy
Herschel 0