Search Publications

Chemical composition of a palomar 12 blue straggler
DOI: 10.1093/mnras/stac842 Bibcode: 2022MNRAS.512.5701P

Pasquini, L.; Bonifacio, P.; Randich, S. +5 more

With the equivalent area of a 16-m telescope, ESPRESSO in 4UT mode allows to inaugurate high resolution spectroscopy for solar-type stars belonging to extragalactic globular clusters. We determine the chemical composition of an extragalactic blue straggler (BS). The star has a G magnitude of 19.01 and belongs to the globular cluster Pal12, that is…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 0
A Gap at 1 au in the Disk of DI Cha A Revealed by Infrared Interferometry
DOI: 10.3847/1538-4357/ac6dee Bibcode: 2022ApJ...932...79J

Pál, András; Moór, Attila; Ábrahám, Péter +6 more

DI Cha A is K0-type pre-main-sequence star, the brightest component of a quadruple stellar system. Here we report on a detailed study of this star based on archival VLTI/MIDI and VLTI/PIONIER infrared interferometric observations, as well as optical-infrared photometric monitoring from ground-based and space-born instruments. We determined the str…

2022 The Astrophysical Journal
AKARI Gaia 0
Cometocentric coordinates of the tail axis of comet 67P/Churyumov-Gerasimenko
DOI: 10.51194/INASAN.2022.7.1.005 Bibcode: 2022INASR...7...30I

Ibragimov, A. A.

In this paper, we consider errors in the measurement of cometocentric coordinates. The sequence of actions for determining the cometocentric coordinates by perspective projection of the image points of the comet onto the orbital plane is given on the example of comet 67P. Conditions are shown that increase the accuracy of determining the angle of …

2022 INASAN Science Reports
Rosetta 0
Similarities and Differences of SARs in Solar Cycle 24
DOI: 10.1007/s11207-022-02076-4 Bibcode: 2022SoPh..297..142C

Li, Ting; Wang, Jingxiu; Chen, Anqin

Solar Cycle 24 is a particularly weak cycle and there are only six super active regions (SARs). Except for NOAA active region (AR) 12192, all other SARs are coronal mass ejection rich (CME-rich) and produced CMEs faster than 1000 kms−1. By studying the similarities and differences between CME-poor SARs and CME-rich SARs in Solar Cycle 2…

2022 Solar Physics
SOHO 0
First Byurakan Spectral Survey. Late-Type Stars. Dwarfs
DOI: 10.52526/25792776-22.69.2-207 Bibcode: 2022CoBAO..69..207G

Gigoyan, K. K.; Gigoyan, K. S.; Kostandyan, G. R. +5 more

A total of 18 lists of the First Byurakan Survey of Late-Type Stars (FBS LTS) were published between 1990 and 2016. The stars were found on FBS low-dispersion spectral plates. A systematic search and selection were carried out on a surface of ∼16 000 deg^2 on almost the whole area of the FBS. Since 2007, all FBS low-resolution spectral plates have…

2022 Communications of the Byurakan Astrophysical Observatory
Gaia 0
X-ray characterisation of the massive galaxy cluster ClG J104803.7+313843 at z = 0.76 with XMM-Newton
DOI: 10.1051/0004-6361/202142313 Bibcode: 2022A&A...660A.112B

Rossetti, M.; Bartalucci, I.; Molendi, S. +6 more

We present the characterisation of the massive cluster ClG J104803.7+313843 at z = 0.76 performed using a serendipitous XMM-Newton observation. High redshift and massive objects represent an ideal laboratory to benchmark our understanding of how clusters form and assembly formation is mainly driven by gravity. Leveraging the high throughput of XMM…

2022 Astronomy and Astrophysics
XMM-Newton 0
X-ray investigation of the X-ray source 1RXS J121902.7-630910 with Suzaku
DOI: 10.1016/j.asr.2022.07.076 Bibcode: 2022AdSpR..70.3263D

Bakis, Hicran; Raycheva, Nergis C.; Sezer, Aytap +1 more

We present a study of the unidentified X-ray source 1RXS J121902.7-630910 based on Suzaku X-ray Imaging Spectrometer observation. We aim at clarifying the nature of the emission from 1RXS J121902.7-630910. We found that the spectrum is well represented by a thermal plasma model with an electron temperature of kTe ∼ 3.7 keV, the upper li…

2022 Advances in Space Research
Suzaku 0
Galactic cosmic ray transport in inner heliosphere: Study with ion chamber and neutron monitor data for 1936-2006
DOI: 10.1016/j.asr.2021.09.017 Bibcode: 2022AdSpR..70.2658A

Modzelewska, R.; Ahluwalia, H. S.; Gololobov, P. Yu.

Galactic cosmic ray (GCR) solar diurnal variation data recorded by shielded ion chambers at Cheltenham/Fredericksburg (CH-IC) and Yakutsk (Yak-IC) are corrected for diurnal temperature variation in upper atmosphere and used to calculate the ratio α of GCR free paths normal (λ) and parallel (λ||) to mean interplanetary magnetic field (I…

2022 Advances in Space Research
Ulysses 0
Solar Photospheric Magnetic Fields, Coronal Mass Ejections, and Type II Radio Bursts in Cycles 23 and 24
DOI: 10.1134/S1063772922080017 Bibcode: 2022ARep...66..579B

Bilenko, I. A.

We consider the events of type II radio bursts (RBII) in the decametric and hectometric ranges from 1 to 16 MHz and the dependence of the parameters of associated coronal mass ejections (CMEs) on the background characteristics of the plasma and interplanetary magnetic field (IMF) in the regions where each radio burst was detected in solar cycles 2…

2022 Astronomy Reports
SOHO 0
Correction to: The Psyche Topography and Geomorphology Investigation
DOI: 10.1007/s11214-022-00879-2 Bibcode: 2022SSRv..218....8J

Williams, David A.; Bell, James F.; Jaumann, Ralf +16 more

2022 Space Science Reviews
MEx 0