Search Publications

Intermittent plasma turbulence in the Martian plasma environment
DOI: 10.1007/s41614-023-00141-4 Bibcode: 2024RvMPP...8....3F

Fränz, Markus; Echer, Ezequiel; Franco, Adriane M. S. +1 more

Due to the absence of a global intrinsic magnetic field, Mars presents an induced magnetosphere, which is formed by the interaction between the solar wind and the conductive ionosphere of the planet. In that interaction, plasma boundaries and regions are created. Wave activity is present in the Mars plasma environment, and as consequence of non-li…

2024 Reviews of Modern Plasma Physics
MEx 0
Ensemble Learning for Stellar Classification and Radius Estimation from Multimodal Data
DOI: 10.1088/1674-4527/ad86a6 Bibcode: 2024RAA....24k5019D

Luo, A. -Li; Kong, Xiao; Li, Xiang-Ru +2 more

Stellar classification and radius estimation are crucial for understanding the structure of the Universe and stellar evolution. With the advent of the era of astronomical big data, multimodal data are available and theoretically effective for stellar classification and radius estimation. A problem is how to improve the performance of this task by …

2024 Research in Astronomy and Astrophysics
Gaia 0
Spectral aging analysis of the 3C 219 double-double radio galaxy
DOI: 10.1051/0004-6361/202450897 Bibcode: 2024A&A...691A..76W

Jamrozy, M.; Wolnik, K.; Jurusik, W.

Context. Double-double radio galaxies are characterized by intermittent jet-formation activity. The exact reasons for this behavior are not yet fully understood. Studying these objects and their environment allows us to find common characteristics and compare them with the general population of radio galaxies. 3C 219 is a well-known and thoroughly…

2024 Astronomy and Astrophysics
eHST 0
A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey
DOI: 10.1051/0004-6361/202452075 Bibcode: 2024A&A...692A.231H

Paunzen, E.; Bernhard, K.; Hümmerich, S.

Context. The magnetic chemically peculiar Ap stars exhibit an extreme spread of rotational velocities, the cause of which is not clearly understood. Ap stars with rotation periods of 50 days or longer are know as super-slowly rotating Ap (ssrAp) stars. Photometrically variable Ap stars are commonly termed α2 Canum Venaticorum (ACV) vari…

2024 Astronomy and Astrophysics
Gaia 0
Spectroscopic Study of Heating Distributions and Mechanisms Using Hinode/EIS
DOI: 10.3847/1538-4357/ad7def Bibcode: 2024ApJ...975..289I

Hara, Hirohisa; Ishigami, Shun; Oba, Takayoshi

Heating distributions along coronal loops are obtained from spectroscopic data with the Hinode/EUV Imaging Spectrometer. The loop half-lengths L half are in the range of 24–107 Mm for our analysis of 18 loops. By using the analytical approximations to 1D hydrostatic numerical calculations of electron temperature T e (s) and …

2024 The Astrophysical Journal
Hinode 0
Measuring 60 pc-scale Star Formation Rate of the Nearby Seyfert Galaxy NGC 1068 with ALMA, HST, VLT/MUSE, and VLA
DOI: 10.3847/1538-4357/ad6312 Bibcode: 2024ApJ...974..243N

Saito, Toshiki; Nakanishi, Kouichiro; Ikarashi, Soh +7 more

The star formation rate (SFR) is a fundamental parameter for describing galaxies and inferring their evolutionary course. H II regions yield the best measure of instantaneous SFR in galaxies, although the derived SFR can have large uncertainties depending on tracers and assumptions. We present an SFR calibration for the entire molecular gas disk o…

2024 The Astrophysical Journal
eHST 0
Strong Localized Pumping of Water Vapor to High Altitudes on Mars During the Perihelion Season
DOI: 10.1029/2023GL107224 Bibcode: 2024GeoRL..5107224B

Aoki, S.; Vandaele, A. C.; Daerden, F. +18 more

Here we present water vapor vertical profiles observed with the ExoMars Trace Gas Orbiter/Nadir and Occultation for MArs Discovery instrument during the perihelion and Southern summer solstice season (LS = 240°-300°) in three consecutive Martian Years 34, 35, and 36. We show the detailed latitudinal distribution of H2O at tan…

2024 Geophysical Research Letters
ExoMars-16 0
Discovery of small ultra-short-period planets orbiting Kepler KG dwarfs with GPU phase folding and deep learning
DOI: 10.1093/mnras/stae2155 Bibcode: 2024MNRAS.534.1913W

Ge, Jian; Wang, Kaitlyn; Willis, Kevin +3 more

Of over 5000 exoplanets identified so far, only a few hundred possess sub-Earth radii. The formation processes of these sub-Earths remain elusive, and acquiring additional samples is essential for investigating this unique population. In our study, we employ the GPFC method, a novel GPU phase folding algorithm combined with a convolutional neural …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0
Structural study of graben within the Margaritifer Terra region of Mars
DOI: 10.1016/j.pss.2024.105840 Bibcode: 2024P&SS..24105840B

Dasgupta, Dipayan; Kundu, Abhik; Basu, Supratik +1 more

The surface of Mars preserves a variety of structural and geomorphic features such as wrinkle ridges, graben, lobate scarps, impact basins, paleochannels etc., which owe their origin to endogenic processes of deformation as well as meteorite impacts. Graben, which form in extensional stress regimes, are one of the most common structural features i…

2024 Planetary and Space Science
MEx 0
North-PHASE: studying periodicity, hot spots, accretion stability, and early evolution in young stars in the Northern hemisphere
DOI: 10.1093/mnras/stae1588 Bibcode: 2024MNRAS.532.2108S

Mendigutía, I.; Garufi, A.; Ábrahám, P. +17 more

We present the overview and first results from the North-PHASE Legacy Survey, which follows six young clusters for five years, using the 2 deg$^2$ FoV of the JAST80 telescope from the Javalambre Observatory (Spain). North-PHASE investigates stellar variability on time-scales from days to years for thousands of young stars distributed over entire c…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0