Search Publications

New Interstellar Extinction Maps Based on Gaia and Other Sky Surveys
DOI: 10.1134/S1063773723110026 Bibcode: 2023AstL...49..673G

Savchenko, S. S.; Gontcharov, G. A.; Il'in, V. B. +5 more

We present new three-dimensional (3D) interstellar extinction maps in the $V$ and Gaia $G$ filters within 2 kpc of the Sun, a 3D differential extinction (dust spatial distribution density) map along lines of sight in the same space, a 3D map of variations in the ratio of the extinctions in the $V$ and Gaia $G$ filters within 800 pc of the Sun, and…

2023 Astronomy Letters
Gaia 3
Predicting convective blueshift and radial-velocity dispersion due to granulation for FGK stars
DOI: 10.1093/mnras/stad2393 Bibcode: 2023MNRAS.525.3344D

Chaplin, W. J.; Meunier, N.; Dalal, S. +2 more

To detect Earth-mass planets using the Doppler method, a major obstacle is to differentiate the planetary signal from intrinsic stellar variability (e.g. pulsations, granulation, spots, and plages). Convective blueshift, which results from small-scale convection at the surface of Sun-like stars, is relevant for Earth-twin detections as it exhibits…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
Polarized Light from Accreting Low Mass X-Ray Binaries
DOI: 10.1134/S1063772923140044 Bibcode: 2023ARep...67S.151C

Capitanio, F.; Farinelli, R.; Fabiani, S. +5 more

Thanks to IXPE, the X-ray spectro-polarimeter launched at the end of 2021, X-ray polarimetry has finally become an extraordinary tool in investigating the physics of accretion in low mass X-ray binaries. Similarly to what happened with gravitational waves, X-ray polarimetry would play a new complementary but at the same time fundamental role in th…

2023 Astronomy Reports
INTEGRAL 3
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images
DOI: 10.1007/s11207-023-02183-w Bibcode: 2023SoPh..298...92S

Berghmans, David; Rachmeler, Laurel A.; West, Matthew J. +5 more

We present the SWAP Filter: an azimuthally varying, radial normalizing filter specifically developed for EUV images of the solar corona, named for the Sun Watcher with Active Pixels and Image Processing (SWAP) instrument on the Project for On-Board Autonomy 2 (PROBA2) spacecraft. We discuss the origins of our technique, its implementation and key …

2023 Solar Physics
PROBA-2 3
Gaia colour-magnitude diagrams of young open clusters. Identification in the UBC catalogue and comparison between manual and automated analyses
DOI: 10.1051/0004-6361/202244933 Bibcode: 2023A&A...675A..19N

de Burgos, A.; Negueruela, I.

Context. Automated analyses of Gaia astrometric data have led to the discovery of many new high-quality open cluster candidates. When a good determination of their parameters is available, these objects become excellent tools for investigating the properties of our Galaxy.
Aims: We explore whether young open clusters can be readily identified…

2023 Astronomy and Astrophysics
Gaia 3
A New Tool for Understanding the Solar Wind-Venus Interaction: Three-dimensional Multifluid MHD Model
DOI: 10.3847/1538-4357/acba88 Bibcode: 2023ApJ...945...91D

Zhang, Tielong; Yao, Zhonghua; Dang, Tong +5 more

In this paper, we present a new tool to investigate the interaction of the solar wind with Venus with the approach of a global multifluid magnetohydrodynamics (MHD) model. The continuity, momentum, and energy equations for H+, O+, ${{\rm{O}}}_{2}^{+}$ , and ${\mathrm{CO}}_{2}^{+}$ are solved self-consistently together with Fa…

2023 The Astrophysical Journal
VenusExpress 3
Sequential Remote Brightenings and Co-spatial Fast Downflows during Two Successive Flares
DOI: 10.3847/1538-4357/ace319 Bibcode: 2023ApJ...953..172W

Cheng, X.; Ding, M. D.; Li, C. +2 more

Remote brightenings often appear at the outskirts of the active regions of solar eruptive events. Nevertheless, their origin remains to be ascertained. In this study, we report imaging and spectroscopic observations of sequential remote brightenings with a combination of observations from the Hα Imaging Spectrograph on board the Chinese Hα Solar E…

2023 The Astrophysical Journal
Hinode 3
NIRwave: A wave-turbulence-driven solar wind model constrained by PSP observations
DOI: 10.1051/0004-6361/202245009 Bibcode: 2023A&A...672A..64S

Güdel, M.; Boro Saikia, S.; Bartel, M. +2 more


Aims: We generate a model description of the solar wind based on an explicit wave-turbulence-driven heating mechanism, and constrain our model with observational data.
Methods: We included an explicit coronal heating source term in the general 3D magnetohydrodynamic code NIRVANA to simulate the properties of the solar wind. The adapted h…

2023 Astronomy and Astrophysics
Ulysses 3
The Transition Region of Solar Flare Loops
DOI: 10.3847/1538-4357/aca8a9 Bibcode: 2023ApJ...943..120G

Antiochos, Spiro K.; Young, Peter R.; Gontikakis, Costis

The transition region between the Sun's corona and chromosphere is important to the mass and energy transfer from the lower atmosphere to the corona; consequently, this region has been studied intensely with ultraviolet and extreme ultraviolet (EUV) observations. A major result of these studies is that the amount of plasma at low temperatures, <…

2023 The Astrophysical Journal
IRIS 3
Investigating the Superorbital Modulations in 4U 1909 + 07, IGR J16418-4532, and IGR J16479-4514 with Swift XRT, BAT, and NuSTAR Observations
DOI: 10.3847/1538-4357/acbc19 Bibcode: 2023ApJ...948...45I

Pottschmidt, Katja; Corbet, Robin H. D.; Coley, Joel B. +2 more

A puzzling variety of superorbital modulations has been discovered in several supergiant high mass X-ray binaries (sgHMXBs). To investigate the mechanisms driving these superorbital modulations, we have analyzed long-term Neil Gehrels Swift Observatory (Swift) Burst Alert Telescope (BAT) observations of three sgHMXBs: 4U 1909 + 07, IGR J16418-4532…

2023 The Astrophysical Journal
INTEGRAL XMM-Newton 3