Search Publications

Hunting for overlooked eccentric eclipsing binaries from ASAS-3 survey
DOI: 10.1016/j.newast.2022.101875 Bibcode: 2022NewA...9701875K

Khalikova, A. V.; Gaynullina, E. R.; Serebryanskiy, A. V.

We present the results of searching for new candidates of eclipsing binaries with eccentric orbits in the ASAS Catalog of Variable Stars (ACVS) using publicly available data from the All Sky Automated Survey (ASAS) and the Transiting Exoplanet Survey Satellite (TESS). Unsupervised machine learning techniques were applied to find anomalies among th…

2022 New Astronomy
Gaia 0
Characterising the orbit and circumstellar environment of the high-mass binary MWC 166 A
DOI: 10.1051/0004-6361/202243957 Bibcode: 2022A&A...665A.146Z

Mérand, Antoine; Monnier, John D.; Lanthermann, Cyprien +13 more

Context. Stellar evolution models are highly dependent on accurate mass estimates, especially for highly massive stars in the early stages of stellar evolution. The most direct method for obtaining model-independent stellar masses is derivation from the orbit of close binaries.
Aims: Our aim was to derive the first astrometric plus radial vel…

2022 Astronomy and Astrophysics
Gaia 0
A novel method for lunar elemental abundance estimation using Chandrayaan-2 class and Chandrayaan-1 M3 data
Bibcode: 2022cosp...44..282B

Bhatt, Megha; Bhardwaj, Anil; Narendranath, Shyama +3 more

We report the first employment of the Chandryaan-2 Large Area Soft X-ray Spectrometer (CLASS) data [1] from Chandrayaan-2 mission as ground truth to estimate SiO2, Al2O3, and MgO for understanding the petrological characteristics of the Moon. The algorithm uses multivariate regression between CLASS derived elemental abundances from selected region…

2022 44th COSPAR Scientific Assembly. Held 16-24 July
Chandrayaan-1 0
Kinematic Classification of Coronal Mass Ejections in LASCO C3 Field of View
DOI: 10.5303/JKAS.2022.55.3.67 Bibcode: 2022JKAS...55...67J

Moon, Yong-Jae; Lee, Harim; Cho, Il-Hyun +2 more

In this study, we perform a statistical investigation of the kinematic classification of 4264 coronal mass ejections (CMEs) from 1996 to 2015 observed by SOHO/LASCO C3. Using the constant acceleration model, we classify these CMEs into three groups: deceleration, constant velocity, and acceleration motion. For this, we devise three different class…

2022 Journal of Korean Astronomical Society
SOHO 0
Plasma dynamics in the flaring loop observed by RHESSI
DOI: 10.1051/0004-6361/202039598 Bibcode: 2022A&A...659A..60M

Kołomański, S.; Mrozek, T.; Falewicz, R. +1 more

Context. Hard X-rays (HXRs) contain the most direct information about the non-thermal electron population in solar flares. The approximation of the HXR emission mechanism (bremsstrahlung), known as the thick-target model, is well developed. It allows one to diagnose the physical conditions within a flaring structure. The thick-target model predict…

2022 Astronomy and Astrophysics
SOHO 0
UGPS J194310+183851: an unusual optical and X-ray faint cataclysmic variable?
DOI: 10.1093/mnras/stac1718 Bibcode: 2022MNRAS.514.6002M

Maccarone, T. J.; Cooper, W. J.; Lucas, P. W. +7 more

The growing number of multi-epoch optical and infrared sky surveys are uncovering unprecedented numbers of new variable stars, of an increasing number of types. The short interval between observations in adjacent near-infrared filters in the UKIDSS Galactic Plane Survey (UGPS) allows for the discovery of variability on the time-scale of minutes. W…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 0
Observaciones del remanente de supernova G296.5+10.0 con el satélite XMM-Newton
Bibcode: 2022BAAA...63..152E

Combi, J. A.; Eppens, L. K.; Reynoso, E. M.

G296.5+10.0 is a 90' × 65'-size supernova remnant (SNR) that displays a bilateral distribution in the radio band with the symmetry axis perpendicular to the Galactic Plane. The remnant shows two emission peaks at the South-East and South-West of the radio shell. In addition, the EXOSAT instrument detected an extended X-ray plasma with an axisymmet…

2022 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
XMM-Newton 0
Mineralogical and Morphological Investigation of Butterfly-Shaped Unnamed Crater Using Datasets from Recent Lunar Missions
Bibcode: 2022LPICo2678.1330N

Pathak, S.; Bhattacharya, S.; Naik, S. S. +3 more

Mineralogical and morphological analyses of an unnamed-butterfly-shaped crater have been studied using Chandrayaan-2 IIRS and other data sets.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 0
Terrestrial Martian analogues from the Indian subcontinent: Implications for hydrological activity on Mars
DOI: 10.1016/j.icarus.2022.115118 Bibcode: 2022Icar..38515118C

Chavan, Anil; Bhandari, Subhash; Bhore, Vivek

Martian geology and surface geomorphic features are grouped under Noachian, Hesperian, and Amazonian eras, based on the crater retention ages and resurfacing ages by crater densities. Comparing the similarities and differences between Martian landforms and their terrestrial analogues promotes an understanding of how surface processes operated on b…

2022 Icarus
MEx 0
Possibilities of velocity field analysis from Hinode SOT/SP data
DOI: 10.1515/astro-2021-0026 Bibcode: 2022OAst...30..203M

Mozharovsky, Sergei G.

The possibility of analyzing the line of sight (LOS) velocity and its gradient at each point of the Hinode SOT/SP maps using bisector analysis is revealed. A technique for obtaining such gradient is described. To estimate the velocity gradient, it is necessary to know both the velocity value and the layer height to which the bisector point is resp…

2022 Open Astronomy
Hinode 0