Results 51 to 60 of about 72 (61)

Multi-Observatory Research of Young Stellar Energetic Flares (MORYSEF): X-Ray-flare-related Phenomena and Multi-epoch Behavior

open access: yesThe Astrophysical Journal
The most powerful stellar flares driven by magnetic energy occur during the early pre-main-sequence (PMS) phase. The Orion Nebula represents the nearest region populated by young stars, showing the greatest number of flares accessible to a single ...
Konstantin V. Getman   +10 more
doaj   +1 more source

Probing the Stellar Populations and Star Formation History of Early-type Galaxies at 0 < z < 1.1 in the Rest-frame Ultraviolet

open access: yesThe Astrophysical Journal
We measure the evolution of the rest-frame near-ultraviolet (NUV)− V colors for early-type galaxies in clusters at 0 < z < 1.1 using data from the Hyper Suprime-Cam Subaru Strategic Program, CFHT Large Area U -band Deep Survey, and local Sloan Digital ...
Sadman S. Ali   +8 more
doaj   +1 more source

The First Exploration of the Correlations Between WISE 12 μm and CO Emission in Early-type Galaxies

open access: yesThe Astrophysical Journal
We present the analysis of a comprehensive sample of 352 early-type galaxies using public data, to investigate the correlations between CO luminosities and mid-infrared luminosities observed by Wide-field Infrared Survey Explorer.
Yang Gao   +12 more
doaj   +1 more source

A Flare-related Decimetric Type-IV Radio Burst Induced by the X2 Radiation of Electron Cyclotron Maser Emission

open access: yesThe Astrophysical Journal Letters
The radiation mechanism of decimetric wideband and pulsating radio bursts from the Sun (in terms of decimetric type-IV (t-IVdm) burst) and other flaring stars is a long-standing problem.
Maoshui Lv   +11 more
doaj   +1 more source

A Long-duration Superflare on the K Giant HD 251108

open access: yesThe Astrophysical Journal
Many giant stars are magnetically active, which causes rotational variability, chromospheric emission lines, and X-ray emission. Large outbursts in these emission features can set limits on the magnetic field strength and thus constrain the mechanism of ...
Hans Moritz Günther   +12 more
doaj   +1 more source

Do Young Suns Produce Frequent, Massive CMEs? Results from Five-year Dedicated Optical Observations of EK Draconis and V889 Hercules

open access: yesThe Astrophysical Journal
We report results from a five-year (132-night) dedicated observational campaign targeting two nearby young solar-type stars, EK Draconis (∼50–125 Myr age) and V889 Hercules (∼30 Myr age), using the 3.8 m Seimei Telescope and Transiting Exoplanet Survey ...
Kosuke Namekata   +6 more
doaj   +1 more source

The Photometric Variability and Spectrum of the Hot Post-AGB Star IRAS 21546+4721

open access: yesGalaxies
We present the results of photometric and spectroscopic observations of a poorly studied B-type supergiant with infrared excess, the hot post-AGB star IRAS 21546+4721.
Natalia Ikonnikova   +2 more
doaj   +1 more source

Ionization Sources of the Local Interstellar Clouds: Two B Stars, Three White Dwarfs, and the Local Hot Bubble

open access: yesThe Astrophysical Journal
The dominant sources of photoionizing radiation in the extreme-ultraviolet (EUV) incident on the exterior of the local interstellar clouds include two nearby early B-type stars, ϵ CMa (124 ± 2 pc) and β CMa (151 ± 5 pc), three hot dwarfs, and the Local ...
J. Michael Shull   +3 more
doaj   +1 more source

Ultraviolet Radiation and Neutrinos: Two Messengers from CCSNe in the CSM Scenario

open access: yesThe Astrophysical Journal
Massive stars (>8 M _⊙ ) often undergo intense mass loss through winds or eruptive events in the final stages of their evolution, leading to the formation of a dense circumstellar medium (CSM). This material, expelled months to years before core collapse,
Silvia Gagliardini   +6 more
doaj   +1 more source

Asymmetries and Circumstellar Interaction in the Type II SN 2024bch

open access: yesThe Astrophysical Journal
We present a comprehensive multi-epoch photometric and spectroscopic study of SN 2024bch, a nearby (19.9 Mpc) Type II supernova (SN) with prominent early high-ionization emission lines.
Jennifer E. Andrews   +31 more
doaj   +1 more source

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