Results 41 to 50 of about 4,002,507 (183)
Chemical and kinematical evolution in nearby dwarf spheroidal galaxies [PDF]
Dwarf spheroidal (dSph) galaxies are the least massive and luminous objects known to exist. These galaxies are often considered as the fossil building blocks of massive systems predicted by some cosmological models.
Koch, Andreas
core +1 more source
The ORCA‐TWIN qCMOS Experiment I. Science Case and Commissioning at Calar Alto Observatory
ABSTRACT We describe a pilot study to explore a new generation of fast and low noise CMOS image sensors for time domain astronomy, using two remote telescopes with a baseline of 1635 km. The experiment involves direct imaging with novel qCMOS image sensor technology that combines fast readout with sub‐electron readout noise.
Martin M. Roth +20 more
wiley +1 more source
Rising Near-ultraviolet Spectra in Stellar Megaflares
Flares from M dwarf stars can attain energies up to 10 ^4 times larger than solar flares but are generally thought to result from similar processes of magnetic energy release and particle acceleration.
Adam F. Kowalski +7 more
doaj +1 more source
The genus Chiropodomys has seen no new species described since the 1980s. Through integrated morphological and molecular analysis, a specimen from Yunnan, China, is identified as a distinct new species, C. wandingensis sp. nov., supported by significant genetic divergence from its closest relatives.
Yi‐shun Qian +3 more
wiley +1 more source
Flaring Activity for Low-mass Stars in the β Pictoris Moving Group
Stellar flares from K and M dwarfs release panchromatic radiation characterized by a significantly higher brightness temperature (∼9–20 kK) than the star. The increased frequency of magnetic activity on young low-mass stars results in the energy released
Jordan N. Ealy +3 more
doaj +1 more source
Searching for Rotational X‐Ray Modulation on TIC 277539431
ABSTRACT TIC 277539431, a fast rotating M7 dwarf, was detected to host the highest latitude flare to date at 81°$$ {81}^{{}^{\circ}} $$. Magnetic activity like stellar flares occurring at high latitude indicate occurrence of coronal loops at these latitudes on fully‐convective M dwarfs. In contrast, sunspots usually occur below 30°$$ {30}^{{}^{\circ}} $
Desmond Dsouza +2 more
wiley +1 more source
We present the X-ray quiescent and flaring properties from a unique, 7 days multiwavelength observing campaign on the M1 flare star AU Mic. Combining the XMM-Newton X-ray spectra with the chromospheric line and broadband near-UV (NUV) and optical ...
Yuta Notsu +5 more
doaj +1 more source
The Constraint of Crewed Mars Missions Based on Current Radiation Dose Measurements
Abstract Crewed missions to Mars will be a milestone of future space exploration programs. However, the absence of Earth's magnetic field leaves astronauts directly exposed to unattenuated energetic particles in deep space, primarily galactic cosmic rays (GCRs), resulting in significantly higher radiation levels and enhanced health risks. Understanding
Chao Zhang +4 more
wiley +1 more source
First Temperature Profile of a Stellar Flare Using Differential Chromatic Refraction
We present the first derivation of a stellar flare temperature profile from single-band photometry. Stellar flare DWF 030225.574−545707.45129 was detected in 2015 by the Dark Energy Camera as part of the Deeper, Wider, Faster program. The brightness (Δ m
Riley W. Clarke +7 more
doaj +1 more source
New flare stars and flares of the known ones in Orion
Observations of red dwarf flare stars were initiated in the Abastumani Astrophysical Observatory in 1969 (Kiladze, 1972). Regions rich in red dwarf stars were selected: the area around Orion Trapezium, and the stellar cluster of Pleiades have been chosen ...
R. Natsvlishvili +2 more
semanticscholar +1 more source

