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Highlights from ILEWG LUNEX EuroMoonMars Earth Space Innovation, ArtMoonMars, Space Renaissance & EuroSpaceHub
Bibcode: 2022cosp...44..292F

Foing, Bernard H.

EuroMoonMars is an ILEWG/LUNEX programme in collaboration with space agencies, academia, universities and research institutions and industries. The programme includes research activities for data analysis, instruments tests and development, field tests in MoonMars analogue, pilot projects, training and hands-on workshops, and outreach activities. …

2022 44th COSPAR Scientific Assembly. Held 16-24 July
SMART-1 0
The Precise Individual Masses and Theoretical Stability and Habitability of some Single-lined Spectroscopic Binaries
DOI: 10.52526/25792776-22.69.2-223 Bibcode: 2022CoBAO..69..223A

Abushattal, A. A.; Kraishan, A. F.; Algnamat, B. S. +1 more

Over the past few decades, some Spectroscopic Binaries (SBs) have been resolved using high-resolution techniques. Astrophysics is interested in this subject because we can obtain the mass of each component. By combining a visual solution with a complimentary one, such as the spectroscopic orbit or Edward method, we can determine the individual mas…

2022 Communications of the Byurakan Astrophysical Observatory
Hipparcos 0
X-ray hot spots in the eastern ear of the supernova remnant W 50 and the microquasar SS 433 system
DOI: 10.1093/pasj/psac011 Bibcode: 2022PASJ...74..510H

Katsuda, Satoru; Sato, Toshiki; Uchiyama, Hideki +10 more

We examined the X-ray and radio spatial structure at the eastern ear of the W 50/SS 433 system to clarify a characteristic feature of the termination region of the SS 433 jet, and found that a hot spot ahead of the filament structure, which is considered to be a terminal shock of the SS 433 eastern jet, is clearly different from a single point sou…

2022 Publications of the Astronomical Society of Japan
Gaia XMM-Newton 0
Photometric Study of the Open Cluster NGC 225
DOI: 10.1134/S1990341322010126 Bibcode: 2022AstBu..77...78Y

Carraro, G.; Ikonnikova, N. P.; Yalyalieva, L. N. +2 more

—NGC 225 is a young moderately populated cluster with discrepant age, distance, and color excess estimates reported by different authors. We combine our photometry with the data from large surveys (2MASS, WISE, Pan-STARRS) to derive the parameters of NGC 225 and study the extinction law in the near infrared in the direction of the cluster. We use …

2022 Astrophysical Bulletin
Gaia 0
Formation and Immediate Deformation of a Small Filament Through Intermittent Magnetic Interactions
DOI: 10.1007/s11207-022-01969-8 Bibcode: 2022SoPh..297...56Z

Zhang, Liang; Chen, Yao; Zheng, Ruisheng +4 more

It is generally believed that filament formation involves a process of the accumulation of magnetic energy. However, in this article, we discuss the idea that filaments will not erupt and will only deform when the stored magnetic energy is released gradually. Combining high-quality observations from SolarDynamicsObservatory and other instruments, …

2022 Solar Physics
IRIS 0
Charge-injection Device Imaging of Sirius with Contrast Ratios Greater than 1:26 Million
DOI: 10.1088/1538-3873/ac54c2 Bibcode: 2022PASP..134c4503S

Sawant, Sailee M.; Batcheldor, Daniel

The intrinsic nature of many astronomical objects, such as binary and multiple systems, exoplanets, circumstellar and debris disks, and quasar host galaxies, introduces challenging requirements for observational instrumentation and techniques. In each case, we encounter situations where the light from bright sources hampers our ability to detect s…

2022 Publications of the Astronomical Society of the Pacific
Gaia 0
Method of evaluation of the most probable mean radial velocities of open star clusters
DOI: 10.51194/INASAN.2022.7.3.006 Bibcode: 2022INASR...7..219K

Kovaleva, D. A.; Kalinkin, A. D.; Kondratev, N. E. +1 more

In this article the method of self-consistent estimate of star clusters' average radial velocity by kinematic parameters was proposed. The method is based on convergent point method of probable cluster members determination. By modelling the method validation was held and properties of received estimate depending on a number of cluster parameters …

2022 INASAN Science Reports
Gaia 0
Studying young stellar populations in G345.5+1.5 molecular cloud
DOI: 10.1016/j.newast.2021.101739 Bibcode: 2022NewA...9301739B

Baume, G.; Borissova, J.; Ramirez Alegria, S.

Using different sky surveys, we studied IRAS sources and embedded clusters located in the G345.5+1.5 region. Our analysis comprises multi-wavelength (optical to radio) data, exploited using various methods: photometry, near-infrared spectroscopy for ten stars in the embedded cluster DBS-114, and astrometry. We estimated the main parameters of the …

2022 New Astronomy
Gaia 0
First Global Lunar Magnesium and Aluminum Abundance Maps Derived Using Chandrayaan-1 and Chandrayaan-2 Data
Bibcode: 2022LPICo2678.2253B

Wöhler, C.; Bhatt, M.; Narendranath, S. +3 more

CLASS-derived abundances of Mg and Al were used as ground truth and an empirical multivariate linear regression model developed for M3 global coverage.

2022 53rd Lunar and Planetary Science Conference
Chandrayaan-1 0
Satellite Confirms the Principle of Falling
DOI: 10.1103/Physics.15.94 Bibcode: 2022PhyOJ..15...94B

Brax, Philippe

The MICROSCOPE satellite experiment has tested the equivalence principle with an unprecedented level of precision.

2022 Physics Online Journal
MICROSCOPE 0