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Space Physics: The Need for a Wider Perspective
DOI: 10.3389/fspas.2022.937742 Bibcode: 2022FrASS...9.7742A

André, Mats

We argue that many studies in space physics would benefit from putting a detailed investigation into a wider perspective. Three examples of theoretical and observational studies are given. We argue that space physics should aim to be less of an isolated branch of science. Rather, by putting the scientific space results into a wider perspective the…

2022 Frontiers in Astronomy and Space Sciences
Cluster 1
A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra
DOI: 10.3847/1538-4357/ac83ba Bibcode: 2022ApJ...936..105H

Jin, Chichuan; Yuan, Weimin; Hu, Jingwei +1 more

The X-ray variability of active galactic nuclei (AGN) carries crucial information about the X-ray radiation mechanism. We performed a systematic study of the X-ray short-term (1-100 ks timescale) variability for a large sample of 78 Seyferts with 426 deep XMM-Newton observations. In this paper, we present the time-averaged spectra and rms spectra …

2022 The Astrophysical Journal
XMM-Newton 1
Detailed analysis of an eccentric TESS binary star with solar-type components: TIC 284613090
DOI: 10.1016/j.newast.2022.101860 Bibcode: 2022NewA...9601860A

Aliçavuş, Fahri

Eclipsing binary stars are significant objects for understanding stellar evolution, stellar population synthesis, and galaxy dynamics. Thanks to the increasing number of high-quality photometric data of space observations, the sensitivity of the fundamental astrophysical parameters (mass M, radius R) has risen and this situation has highlighted th…

2022 New Astronomy
Gaia 1
MAXI J1535-571 2017 Outburst Seen by INTEGRAL/SPI and Investigating the Origin of Its Hard Tail
DOI: 10.3847/1538-4357/ac7fff Bibcode: 2022ApJ...935...25R

Jourdain, E.; Roques, J. P.; Rodi, James

On 2017 September 2 MAXI J1535-571 went into outburst and peaked at ~5 Crab in the 2-20 keV energy range. Early in the flare, the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) performed target of opportunity pointings and monitored the source as it transitioned from the hard state to the soft state. Using quasi-simultaneous observatio…

2022 The Astrophysical Journal
INTEGRAL 1
Hydrological History of a Palaeolake and Valley System on the Planetary Dichotomy in Arabia Terra, Mars
DOI: 10.1029/2021JE007152 Bibcode: 2022JGRE..12707152D

Grindrod, P. M.; Davis, J. M.; Balme, M. +2 more

Hundreds of ancient palaeolake basins have been identified and cataloged on Mars, indicating the distribution and availability of liquid water as well as sites of astrobiological potential. Palaeolakes are widely distributed across the Noachian aged terrains of the southern highlands, but Arabia Terra hosts few documented palaeolakes and even fewe…

2022 Journal of Geophysical Research (Planets)
MEx 1
Decoding the Bifurcated Red Giant Branch as a Tracer of Multiple Stellar Populations in the Young Large Magellanic Cloud Cluster NGC 2173
DOI: 10.3847/2041-8213/ac551a Bibcode: 2022ApJ...927L..10K

Zucker, Daniel B.; de Grijs, Richard; Kamath, Devika +1 more

Multiple stellar populations (MPs) representing star-to-star light-element abundance variations are common in nearly all ancient Galactic globular clusters (GCs). Here we provide the strongest evidence yet that the populous, ~1.7 Gyr old Large Magellanic Cloud cluster NGC 2173 also exhibits light-element abundance variations. Thus, our results sug…

2022 The Astrophysical Journal
eHST 1
Anisotropic nonthermal motions in the transition region of solar active regions
DOI: 10.1051/0004-6361/202142285 Bibcode: 2022A&A...660A...3M

Peter, Hardi; Xia, Lidong; Huang, Zhenghua +1 more

Context. We study the nonthermal motions in the transition region of active regions (ARs) using center-to-limb observations of Si IV 1394 Å and 1403 Å lines.
Aims: The aim of this study is to investigate the characteristics of nonthermal motions in the transition region of ARs using the center-to-limb measurement.
Methods: We used Interf…

2022 Astronomy and Astrophysics
IRIS 1
Diffuse Interstellar Bands λ6379, λ6614, and λ6660 in the LAMOST-MRS Spectra
DOI: 10.1088/1674-4527/ac7388 Bibcode: 2022RAA....22h5007W

Luo, A. -Li; Hou, Wen; Zhao, Yong-Heng +2 more

Diffuse interstellar bands (DIBs) have always been a mysterious existence in astronomical research. In this work, we provide more DIB samples to slightly uncover this mystery. With the LAMOST medium-resolution survey (MRS) spectra, we detected three DIBs λ6379, λ6614, and λ6660, obviously superimposed on the spectra of 11,003 stars. These spectra …

2022 Research in Astronomy and Astrophysics
Gaia 1
Radial velocities from far-red spectra of Carina Arm O and early B stars
DOI: 10.1093/mnras/stac2045 Bibcode: 2022MNRAS.515.5993D

Drew, J. E.; Blake-Parsons, F.; Mohr-Smith, M.

Massive O and early B stars are important markers of recent star formation and exert a significant influence on their environments during their short lives via photoionization and winds and when they explode as supernovae. In the Milky Way, they can be detected at great distances but often lie behind large dust columns, making detection at short w…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 1
Locating Red Supergiants in the Galaxy NGC 6822
DOI: 10.3847/1538-3881/ac410e Bibcode: 2022AJ....163...70D

Massey, Philip; Levesque, Emily M.; Neugent, Kathryn F. +1 more

Using archival near-IR photometry, we identify 51 of the K-band brightest red supergiants (RSGs) in NGC 6822 and compare their physical properties with stellar evolutionary model predictions. We first use Gaia parallax and proper motion values to filter out foreground Galactic red dwarfs before constructing a J-K versus K color-magnitude diagram t…

2022 The Astronomical Journal
Gaia 1