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X-ray pulsar HD 49798: a contracting white dwarf with a debris disk?
DOI: 10.1051/0004-6361/202243536 Bibcode: 2022A&A...662A..79C

Chen, Wen-Cong

HD 49798/RX J0648.0C4418 is a peculiar binary including a hot subdwarf of O spectral type and a compact companion in a 1.55 day orbit. Based on the steady spin period derivative Ṗ = (−2.17 ± 0.01) × 10−15 s s−1 , the compact object was thought to be a contracting young white dwarf (WD). However, the X-ray luminosity produced …

2022 Astronomy and Astrophysics
Gaia 3
Solar Minimum Exospheric Neutral Density Near the Subsolar Magnetopause Estimated From the XMM Soft X-Ray Observations on 12 November 2008
DOI: 10.1029/2021JA029676 Bibcode: 2022JGRA..12729676J

Pagani, C.; Kuntz, K. D.; Koutroumpa, D. +3 more

The Earth's magnetosheath and cusps emit soft X-rays due to the charge exchange between highly charged solar wind ions and exospheric hydrogen atoms. The Lunar Environment Heliospheric X-ray Imager and Solar wind Magnetosphere Ionosphere Link Explorer missions are scheduled to image the Earth's dayside magnetosphere system in soft X-rays to invest…

2022 Journal of Geophysical Research (Space Physics)
XMM-Newton 3
Search for an Alien Message to a Nearby Star
DOI: 10.3847/1538-3881/ac9610 Bibcode: 2022AJ....164..221G

Wright, Jason T.; Gillon, Michaël; Burdanov, Artem

If alien probes have colonized the whole galaxy, they could have formed an efficient galactic-scale communication network by establishing direct gravitationally lensed links between neighboring systems. Under this scenario, observing the positions opposite the nearest ecliptic stars represents a promising artifact SETI strategy that could make it …

2022 The Astronomical Journal
Gaia 3
Open clusters with proper motions fully separatedfrom the field stars using Gaia DR2
DOI: 10.1080/20909977.2022.2037817 Bibcode: 2022JAsGe..11..142B

Tadross, A. L.; Badawy, W. A.; Hendy, Y. H. M. +3 more

The study of open star clusters makes us understand a lot about the composition and construction of the Milky Way Galaxy. Thanks to the Gaia DR2 database that helps us to get the genetic members of star clusters using their proper motions and parallaxes, estimating their physical properties in a very accurate way. This study aims to detect the rea…

2022 NRIAG Journal of Astronomy and Geophysics
Gaia 3
On the validity of the spectroscopic age indicators [Y/Mg], [Y/Al], [Y/Si], [Y/Ca], and [Y/Ti] for giant stars
DOI: 10.1093/mnras/stac1183 Bibcode: 2022MNRAS.514.4816K

Abuchaim, Yuri; Kerber, Leandro; Katime Santrich, Orlando J. +1 more

The abundance ratios [Y/Mg], [Y/Al], [Y/Si], [Y/Ca], and [Y/Ti] have been suggested as chemical clocks for solar-metallicity dwarf stars in the field as well as for giant stars in open clusters. To verify this last hypothesis, we derive these abundances ratios of 50 giant stars belonging to seven open clusters. To calculate the abundances, we anal…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Companion mass limits for 17 binary systems obtained with binary differential imaging and MagAO/Clio
DOI: 10.1093/mnras/stac2056 Bibcode: 2022MNRAS.515.4487P

Weinberger, Alycia J.; Close, Laird M.; Males, Jared R. +4 more

Improving direct detection capability close to the star through improved star subtraction and post-processing techniques is vital for discovering new low-mass companions and characterizing known ones at longer wavelengths. We present results of 17 binary star systems observed with the Magellan adaptive optics system (MagAO) and the Clio infrared c…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
The CGM-GRB Study. II. Outflow-Galaxy Connection at z 2-6
DOI: 10.3847/1538-4357/ac408e Bibcode: 2022ApJ...926...63G

Cenko, S. Bradley; Veilleux, Sylvain; Perley, Daniel +4 more

We use a sample of 27 gamma-ray bursts (GRBs) at redshift z = 2-6 to probe the outflows in their respective host galaxies (log(M */M ) ~ 9-11) and search for possible relations between the outflow properties and those of the host galaxies, such as M *, the star formation rate (SFR), and the specific SFR (sSFR). Fi…

2022 The Astrophysical Journal
Gaia eHST 3
A New Period Determination Method for Periodic Variable Stars
DOI: 10.1088/1538-3873/ac9e1b Bibcode: 2022PASP..134k4507X

Li, Bin; Li, Xu-Zhi; Zhu, Qing-Feng +4 more

Variable stars play a key role in understanding the Milky Way and the universe. The era of astronomical big data presents new challenges for quick identification of interesting and important variable stars. Accurately estimating the periods is the most important step to distinguish different types of variable stars. Here, we propose a new method o…

2022 Publications of the Astronomical Society of the Pacific
Gaia 3
Active region and flare ribbon properties associated with X-class flares and CMEs of solar cycle 24
DOI: 10.1007/s10509-022-04061-6 Bibcode: 2022Ap&SS.367...33V

Moon, Y. -J.; Shanmugaraju, A.; Lim, Daye +4 more

The solar eruptive events and their origin are important in the context of forecasting their occurrence and their effects on the space and the earth. In this paper, a set of 45 X-class flare-associated coronal mass ejections (CMEs) and their source region characteristics are analysed. The X-ray flares and white light CMEs were observed by GOES and…

2022 Astrophysics and Space Science
SOHO 3
A multiwavelength study of the flat-spectrum radio quasar NVSS J141922-083830 covering four flaring episodes
DOI: 10.1093/mnras/stac2181 Bibcode: 2022MNRAS.517.5791B

Stalin, C. S.; Kniazev, A.; Buckley, D. A. H. +9 more

We present multiwavelength observations and a model for flat-spectrum radio quasar (FSRQ) NVSS J141922-083830, originally classified as a blazar candidate of unknown type (BCU II object) in the Third Fermi-LAT AGN Catalog. Relatively bright flares (>3 magnitudes) were observed on 2015 February 21 (MJD 57074) and 2018 September 8 (MJD 58369) in …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3