Search Publications

SRG/ART-XC, Swift, NICER, and NuSTAR study of different states of the transient X-ray pulsar MAXI J0903-531
DOI: 10.1051/0004-6361/202141821 Bibcode: 2022A&A...661A..45T

Wilms, Jörn; Doroshenko, Victor; Tsygankov, Sergey S. +6 more

The results of the broadband spectral and timing study of the recently discovered transient X-ray pulsar MAXI J0903-531 in a wide range of luminosities that differ by a factor of ~30 are reported. The observed X-ray spectrum in both states can be described as a classical pulsar-like spectrum consisting of a power law with a high-energy cutoff. We …

2022 Astronomy and Astrophysics
Gaia 3
Tracking of magnetic helicity evolution in the inner heliosphere. A radial alignment study
DOI: 10.1051/0004-6361/202244314 Bibcode: 2022A&A...664L...8A

Richter, I.; Narita, Y.; Hadid, L. Z. +5 more

Context. Magnetic helicity is one of the invariants in ideal magnetohydrodynamics, and its spectral evolution has a substantial amount of information to reveal the mechanism that are behind turbulence in space and astrophysical plasmas.
Aims: The goal of our study is to observationally characterize the magnetic helicity evolution in the inner…

2022 Astronomy and Astrophysics
BepiColombo 3
New Short-Period δ Scuti Stars in OGLE-IV Fields toward the Galactic Bulge
DOI: 10.32023/0001-5237/72.3.1 Bibcode: 2022AcA....72..161P

Soszyński, I.; Udalski, A.; Szymański, M. K. +12 more

We report the classification of 24 puzzling short-period variable stars located in OGLE-IV Galactic bulge fields. The stars are low-amplitude (<0.05 mag) multi-periodic objects with dominant periods between 22 min and 54 min whose type could not have been unambiguously established based on photometry only. A low-resolution spectroscopic follow-…

2022 Acta Astronomica
Gaia 3
Power Anisotropy, Dispersion Signature and Turbulence Diffusion Region in the 3D Wavenumber Domain of Space Plasma Turbulence
DOI: 10.3847/1538-4357/ac8e07 Bibcode: 2022ApJ...939..121L

Verscharen, Daniel; He, Jiansen; Sahraoui, Fouad +4 more

We explore the multifaceted important features of turbulence (e.g., anisotropy, dispersion, and diffusion) in the three-dimensional (3D) wavenumber domain (k , k ⊥,1, k ⊥,2), by employing the k-filtering technique to high-quality measurements of fields and particles from the Magnetospheric Multiscale Mission (MMS)…

2022 The Astrophysical Journal
Cluster 3
Venus' Cloud-Tracked Winds Using Ground- and Space-Based Observations with TNG/NICS and VEx/VIRTIS
DOI: 10.3390/atmos13020337 Bibcode: 2022Atmos..13..337M

Machado, Pedro; Peralta, Javier; Silva, José E. +3 more

Characterizing the wind speeds of Venus and their variability at multiple vertical levels is essential for a better understanding of the atmospheric superrotation, constraining the role of large-scale planetary waves in the maintenance of this superrotation, and in studying how the wind field affects clouds' distribution. Here, we present cloud-tr…

2022 Atmosphere
VenusExpress 3
WASP-35 and HAT-P-30/WASP-51: Reanalysis using TESS and Ground-based Transit Photometry
DOI: 10.3847/1538-3881/ac5b6a Bibcode: 2022AJ....163..208B

Wang, Xiaobin; Gu, Shenghong; Sun, Leilei +3 more

High-precision transit observations provide excellent opportunities for characterizing the physical properties of exoplanetary systems. These physical properties supply many pieces of information for unvealing the internal structure, external atmosphere, and dynamical history of the planets. We present revised properties of the transiting systems …

2022 The Astronomical Journal
Gaia 3
A Search for Analogs of KIC 8462852 (Boyajian's Star): A Second List of Candidates
DOI: 10.3847/1538-3881/ac3416 Bibcode: 2022AJ....163...10S

Schmidt, Edward G.

In data from the Kepler mission, the normal F3V star KIC 8462852 (Boyajian's star) was observed to exhibit infrequent dips in brightness that have not been satisfactorily explained. A previous paper reported the first results of a search for other similar stars in a limited region of the sky around the Kepler field. This paper expands on that sear…

2022 The Astronomical Journal
Gaia 3
Is Fermi 1544-0649 a Misaligned Blazar? Discovering the Jet Structure with Very Long Baseline Interferometry
DOI: 10.3847/1538-4357/ac778c Bibcode: 2022ApJ...934...39S

Zhang, Zhongli; Chen, Wen; Cheng, Xiaopeng +8 more

Fermi J1544-0649 is a transient GeV source first detected during its GeV flares in 2017. Multiwavelength observations during the flaring time demonstrate variability and spectral energy distributions that are typical of a blazar. Other than the flare time, Fermi J1544-0649 is quiet in the GeV band and has looked rather like a quiet galaxy (2MASX J…

2022 The Astrophysical Journal
Gaia 3
Sunspot numbers and proton events in solar cycles 19 to 24
DOI: 10.1016/j.jastp.2022.105891 Bibcode: 2022JASTP.23605891B

Bromage, B. J. I.; Birch, M. J.

In this study we compare the mean annual sunspot numbers for the six most recent solar cycles (19 to 24) with the number of solar energetic proton events occurring in those years. Though most of the individual cycles exhibit quite strong correlations, when they are combined into a generic solar cycle the result is very significant (ρ = 0.98). For …

2022 Journal of Atmospheric and Solar-Terrestrial Physics
SOHO 3
CME-related Large Decreases in the Differential Phase Delay of Tianwen-1 DOR Signals
DOI: 10.3847/2041-8213/aca2a8 Bibcode: 2022ApJ...940L..45H

Liu, Kaijun; Guo, Li; He, Qingbao +2 more

Differential phase delay is calculated for the differential one-way range (DOR) signals transmitted by Tianwen-1, the first Chinese Mars spacecraft that entered into the Mars orbit on 2021 February 10. Large decreases in the differential phase delay are identified in the DOR signals received by ground stations on 2021 March 23 and June 18. The dec…

2022 The Astrophysical Journal
SOHO 3