Search Publications

The impact of the presence of water ice on the analysis of debris disk observations
DOI: 10.1051/0004-6361/202141413 Bibcode: 2022A&A...658A.121S

Wolf, S.; Stuber, T. A.

Context. The analysis of debris disk observations is often based on the assumption of a dust phase composed of compact spherical grains consisting of astronomical silicate. Instead, observations indicate the existence of water ice in debris disks.
Aims: We quantify the impact of water ice as a potential grain constituent in debris disks on th…

2022 Astronomy and Astrophysics
Gaia 3
Selection of the Main Control Parameters for the Dst Index Prediction Model Based on a Layer-wise Relevance Propagation Method
DOI: 10.3847/1538-4365/ac616c Bibcode: 2022ApJS..260....6L

Zhang, J.; Wang, Z.; Li, Y. Y. +8 more

The prediction of the Dst index is an important subject in space weather. It has significant progress with the prevalent applications of neural networks. The selection of input parameters is critical for the prediction model of the Dst index or other space-weather models. In this study, we perform a layer-wise relevance propagation (LRP) method to…

2022 The Astrophysical Journal Supplement Series
Gaia 3
Planet Patrol: Vetting Transiting Exoplanet Candidates with Citizen Science
DOI: 10.1088/1538-3873/ac5de0 Bibcode: 2022PASP..134d4401K

Kostov, Veselin B.; Kuchner, Marc J.; Brande, Jonathan +15 more

NASA's TESS mission yields light curves for tens of millions of stars spread across the entire sky, a data set that will be a challenge to fully exploit without help from citizen scientists. To address this, we launched a new citizen science project, called "Planet Patrol", designed to analyze TESS data on exoplanet and eclipsing binary candidates…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
The 2020 Eclipse of R Aquarii in the Near-infrared: Mid-eclipse Observations of Disk Distress
DOI: 10.3847/1538-4357/ac8a47 Bibcode: 2022ApJ...937...98H

Fekel, Francis C.; Hinkle, Kenneth H.; Lebzelter, Thomas +2 more

The Mira in the bright, dusty, symbiotic binary R Aquarii undergoes eclipses of multiyear duration every ~44 yr by a large, opaque accretion disk. The 2020 eclipse was confirmed by I-band photometry. High-resolution M- and K-band spectra were observed near the midpoint of the eclipse, in 2020 August and September. The 4.5-5.5 µm spectrum dur…

2022 The Astrophysical Journal
Gaia 3
Far-ultraviolet investigation into the galactic globular cluster M30 (NGC 7099): I. Photometry and radial distributions
DOI: 10.1093/mnras/stac242 Bibcode: 2022MNRAS.511.3785M

Zurek, David R.; Kroupa, Pavel; Long, Knox S. +4 more

We present a far-ultraviolet (FUV) study of the globular cluster M30 (NGC 7099). The images were obtained using the Advanced Camera for Surveys (ACS/SBC, F150LP, FUV) and the Wide Field Planetary Camera 2 (WFPC2, F300W, UV) which were both onboard the Hubble Space Telescope. The FUV - UV colour-magnitude diagram (CMD) shows a main sequence (MS) tu…

2022 Monthly Notices of the Royal Astronomical Society
eHST 3
Estimation of Galactic Spiral Density Wave Parameters Based on the Velocities of OB2 Stars from the Gaia EDR3 Catalogue
DOI: 10.1134/S1063773722020025 Bibcode: 2022AstL...48..169B

Bobylev, V. V.; Bajkova, A. T.

We have analyzed the kinematics of 9750 OB2 stars with proper motions and parallaxes selected by Xu et al. from the Gaia EDR3 catalogue. The relative parallax errors for these stars do not exceed 10${%}$. Based on the entire sample of stars, we have found the velocities $(U,V)_{\odot}=(7.17,7.37)±(0.16,0.24)$ km s${}^{-1}$ and the components of th…

2022 Astronomy Letters
Gaia 3
X-ray spectral and timing analysis of the Compton Thick Seyfert 2 galaxy NGC 1068
DOI: 10.1093/mnras/stac2736 Bibcode: 2022MNRAS.517.3341P

Stalin, C. S.; Marchesi, S.; Parker, M. L. +2 more

We present the timing and spectral analysis of the Compton Thick Seyfert 2 active galactic nuclei NGC 1068 observed using NuSTAR and XMM-Newton. In this work for the first time we calculated the coronal temperature ($\rm {kT_{e}}$) of the source and checked for its variation between the epochs if any. The data analysed in this work comprised of (a…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 3
Star Formation Triggered by the Expanding Bubble S111
DOI: 10.3847/1538-4357/ac4258 Bibcode: 2022ApJ...926....4M

Mookerjea, Bhaswati

This paper investigates the impact of radiative and mechanical feedback from O-type stars on their parent molecular clouds and the triggering of formation of a future generation of stars. We study the infrared bubble S111 created by the embedded massive stellar cluster G316.80-0.05. A significant fraction of gas in shells created due to the compre…

2022 The Astrophysical Journal
Herschel 3
Formation of Coronal Mass Ejection and Posteruption Flow of Solar Wind on 2010 August 18 Event
DOI: 10.3847/1538-4357/ac5901 Bibcode: 2022ApJ...929..146S

Slemzin, Vladimir; Goryaev, Farid; Rodkin, Denis

The state of the space environment plays a significant role in the forecasting of geomagnetic storms produced by disturbances of the solar wind (SW). Coronal mass ejections (CMEs) passing through the heliosphere often have a prolonged (up to several days) trail with declining speed, which affects propagation of the subsequent SW streams. We studie…

2022 The Astrophysical Journal
PROBA-2 SOHO 3
Pipeline for the Antarctic Survey Telescope 3-3 in Yaoan, Yunnan
DOI: 10.3389/fspas.2022.897100 Bibcode: 2022FrASS...9.7100S

Wang, Lifan; Castro-Tirado, A. J.; Hu, Lei +5 more

AST3-3 is the third robotic facility of the Antarctic Survey Telescopes (AST3) for transient surveys to be deployed at Dome A, Antarctica. Due to the current pandemic, the telescope has been currently deployed at the Yaoan Observation Station in China, starting the commissioning observation and a transient survey. This article presented a fully au…

2022 Frontiers in Astronomy and Space Sciences
Gaia 3