Search Publications

Evaluating Helium Variations By Modeling Red Giant Branch Bump of Large Magellanic Cluster NGC 1978
DOI: 10.1088/1674-4527/ac46a3 Bibcode: 2022RAA....22c5008J

Li, Cheng-Yuan; Ji, Xin; Deng, Li-Cai

Many evidences show that the Multiple Population (MP) features exist not only in old clusters but also in intermediate-age clusters in the Megallanic Clouds (MCs), which are characterized by star-to-star abundance scatter of several elements, including helium (He). The red giant branch bump (RGBB)'s photometric properties are proved to be related …

2022 Research in Astronomy and Astrophysics
eHST 2
Optical microflares in LS I +61 303 and the search for their multiwavelength counterpart
DOI: 10.1051/0004-6361/202243318 Bibcode: 2022A&A...662A..27M

Luque-Escamilla, Pedro L.; Martí, Josep; del Ser, Daniel +4 more

Context. Stellar sources of gamma rays are one of the front lines in modern astrophysics whose understanding can benefit from observational tools not originally designed for their study.
Aims: We take advantage of the high precision photometric capabilities of present-day space facilities to obtain a new perspective on the optical behavior of…

2022 Astronomy and Astrophysics
Gaia 2
Compact and Variable Radio Emission from an Active Galaxy with Supersoft X-Ray Emission
DOI: 10.3847/1538-4357/ac80ba Bibcode: 2022ApJ...935..115Y

Li, Di; Liu, Daizhong; Yang, Lei +15 more

RX J1301.9+2747 is a unique active galaxy with a supersoft X-ray spectrum that lacks significant emission at energies above 2 keV. In addition, it is one of few galaxies displaying quasiperiodic X-ray eruptions that recur on a timescale of 13-20 ks. We present multiepoch radio observations of RX J1301.9+2747 using GMRT, Very Large Array (VLA), and…

2022 The Astrophysical Journal
Gaia 2
Globular Cluster as Indicators of Galactic Evolution
DOI: 10.1134/S1063772922030015 Bibcode: 2022ARep...66..191A

Pilipenko, S. V.; Arkelyan, N. R.

We have studied the system of globular clusters (GCs) that formed in other galaxies and eventually accreted onto the Milky Way. Thus, the samples of GCs belonging to different tidal streams, obtained on the basis of the latest data from the GAIA observatory, were taken from the literature. We measured the anisotropy of the distribution of these GC…

2022 Astronomy Reports
Gaia 2
Catalogs of Solar Proton Events as a Tool for Studying Space Weather
DOI: 10.1134/S001095252203008X Bibcode: 2022CosRe..60..151V

Vlasova, N. A.; Bazilevskaya, G. A.; Ginzburg, E. A. +8 more

Distinguishing features of a series of solar proton event (SPE) catalogs for the 20th-24th cycles of solar activity are described. The results of a comparative analysis of the 23rd and 24th cycles of solar activity performed according to the data of a series of SPE catalogs are presented. The opportunities provided by SPE catalogs for studying spa…

2022 Cosmic Research
SOHO 2
Multiwavelength Observations of MWC 297: Constraints on Disk Inclination and Mass Outflow
DOI: 10.3847/1538-4357/ac94c4 Bibcode: 2022ApJ...941..189V

Vacca, William D.; Sandell, Göran

MWC 297 is a young, early-type star driving an ionized outflow and surrounded by warm, entrained dust. Previous analyses of near- and mid-IR interferometric images suggest that the emission at these wavelengths arises from a compact accretion disk with a moderate (i < 40°) inclination. We have obtained 5-40 µm images of MWC 297 with FORCA…

2022 The Astrophysical Journal
Herschel 2
ArTéMiS imaging of the filamentary infrared dark clouds G1.75-0.08 and G11.36+0.80: Dust-based physical properties of the clouds and their clumps
DOI: 10.1051/0004-6361/202243027 Bibcode: 2022A&A...667A..90M

André, Ph.; Miettinen, O.; Mattern, M.

Context. Filamentary infrared dark clouds (IRDCs) are a useful class of interstellar clouds for studying the cloud fragmentation mechanisms on different spatial scales. Determination of the physical properties of the substructures in IRDCs can also provide useful constraints on the initial conditions and early stages of star formation, including t…

2022 Astronomy and Astrophysics
Herschel 2
Orbital period changes in IO Cep, IM Cep and TX Ari: Path to masses of distant components
DOI: 10.1016/j.newast.2021.101754 Bibcode: 2022NewA...9301754B

Bakış, V.; Eker, Z.; Bakış, H. +7 more

Three Algol-type binary systems (IO Cep, IM Cep and TX Ari) showing cyclic orbital period changes are studied. The combination of time of minimum data from the ground-based observations together with high precision photometric data from the TESS satellite enabled us to estimate the basic light curve elements of binary systems and mass functions fo…

2022 New Astronomy
Gaia 2
A Parametric Study of Performance of Two Solar Wind Velocity Forecasting Models During 2006-2011
DOI: 10.1029/2022SW003069 Bibcode: 2022SpWea..2003069K

Srivastava, Nandita; Kumar, Sandeep

There is an increasing need for the development of a robust space weather forecasting framework. State-of-the-art MHD space weather forecasting frameworks are based upon the Potential Field Source Surface (PFSS) and Schatten Current Sheet (SCS) extrapolation models for the magnetic field using synoptic magnetograms. These models create a solar win…

2022 Space Weather
SOHO 2
Plasma Diagnostics in the Era of Integral Field Spectroscopy
DOI: 10.3390/galaxies10010030 Bibcode: 2022Galax..10...30U

Ueta, Toshiya

To understand the physical conditions of various gaseous systems, plasma diagnostics must be performed properly. To that end, it is equally important to have extinction correction performed properly, even before performing plasma diagnostics. This means that the physical conditions of the target sources—the very quantities to be derived via plasma…

2022 Galaxies
eHST 2