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Density and Temperature of the Upper Mesosphere and Lower Thermosphere of Mars Retrieved From the OI 557.7 nm Dayglow Measured by TGO/NOMAD
DOI: 10.1029/2022JE007206 Bibcode: 2022JGRE..12707206A

Aoki, S.; Vandaele, A. C.; Daerden, F. +15 more

The upper mesosphere and lower thermosphere of Mars (70-150 km) is of high interest because it is a region affected by climatological/meteorological events in the lower atmosphere and external solar forcing. However, only a few measurements are available at this altitude range. OI 557.7 nm dayglow emission has been detected at these altitudes by t…

2022 Journal of Geophysical Research (Planets)
ExoMars-16 10
Multiband photometry of Martian Recurring Slope Lineae (RSL) and dust-removed features at Horowitz crater, Mars from TGO/CaSSIS color observations
DOI: 10.1016/j.pss.2022.105443 Bibcode: 2022P&SS..21405443M

Pajola, M.; Cremonese, G.; Thomas, N. +12 more

Recurring Slope Lineae (RSL) are narrow, dark streaks typically lengthening down Martian steep slopes during warm seasons, fading during the cold ones and regularly recurring every Martian year. Their origin is still debated. Although initially interpreted as possible flows of seeping water, either coming from a subsurface aquifer or through atmos…

2022 Planetary and Space Science
ExoMars-16 10
Dust Extinction Law in Nearby Star-resolved Galaxies. II. M33 Traced by Supergiants
DOI: 10.3847/1538-4365/ac63c1 Bibcode: 2022ApJS..260...41W

Gao, Jian; Ren, Yi; Chen, Bingqiu +1 more

The dust extinction curves toward individual sight lines in M33 are derived for the first time with a sample of reddened O-type and B-type supergiants obtained from the Local Group Galaxies Survey (LGGS). The observed photometric data are obtained from the LGGS, PS1 Survey, UKIRT, PHATTER Survey, Galaxy Evolution Explorer, Swift/UVOT, and XMM-SUSS…

2022 The Astrophysical Journal Supplement Series
XMM-Newton eHST 10
The eROSITA Final Equatorial-Depth Survey (eFEDS). The first archetypal quasar in the feedback phase discovered by eROSITA
DOI: 10.1051/0004-6361/202141092 Bibcode: 2022A&A...661A...9B

Silverman, J. D.; Georgakakis, A.; Salvato, M. +18 more

Theoretical models of the co-evolution of galaxies and active galactic nuclei (AGNs) ascribe an important role in the feedback process to a short, luminous, obscured, and dust-enshrouded phase during which the accretion rate of the supermassive black hole is expected to be at its maximum and the associated AGN-driven winds are also predicted to be…

2022 Astronomy and Astrophysics
Herschel 10
The Accretion Process in the DQ Tau Binary System
DOI: 10.3847/1538-4357/ac4790 Bibcode: 2022ApJ...928...81F

Ábrahám, P.; Kóspál, Á.; Fiorellino, E. +1 more

Mass accretion from the circumstellar disk onto the protostar is a fundamental process during star formation. Measuring the mass accretion rate is particularly challenging for stars belonging to binary systems, because it is often difficult to discriminate which component is accreting. DQ Tau is an almost equal-mass spectroscopic binary system whe…

2022 The Astrophysical Journal
Gaia 10
Three-dimensional magnetic fields of molecular clouds
DOI: 10.3389/fspas.2022.940027 Bibcode: 2022FrASS...9.0027T

Tahani, Mehrnoosh

To investigate the role of magnetic fields in the evolution of the interstellar medium, formation and evolution of molecular clouds, and ultimately the formation of stars, their three-dimensional (3D) magnetic fields must be probed. Observing only one component of magnetic fields (along the line of sight or parallel to the plane of the sky) is ins…

2022 Frontiers in Astronomy and Space Sciences
Gaia 10
Binaries with Possible Compact Components Discovered from the LAMOST Time-domain Survey of Four K2 Plates
DOI: 10.3847/1538-4357/ac8f29 Bibcode: 2022ApJ...938...78L

Liu, Jifeng; Zhang, Haotong; Wang, Song +4 more

Time-domain spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) can provide accurate and high-cadence radial velocities (RVs). In this work, we search for binaries with compact components with the RV monitoring method by using the LAMOST time-domain survey of four K2 plates. Three binary systems including…

2022 The Astrophysical Journal
Gaia 10
A strong H opacity signal in the near-infrared emission spectrum of the ultra-hot Jupiter KELT-9b
DOI: 10.1051/0004-6361/202244533 Bibcode: 2022A&A...668L...1J

Schlawin, E.; Pino, L.; Désert, J. -M. +11 more

We present the analysis of a spectroscopic secondary eclipse of the hottest transiting exoplanet detected to date, KELT-9b, obtained with the Wide Field Camera 3 aboard the Hubble Space Telescope. We complement these data with literature information on stellar pulsations and Spitzer/Infrared Array Camera and Transiting Exoplanet Survey Satellite e…

2022 Astronomy and Astrophysics
eHST 10
Discovery of 16 New Members of the Solar Neighborhood Using Proper Motions from CatWISE2020
DOI: 10.3847/1538-3881/ac4713 Bibcode: 2022AJ....163..116K

Meisner, Aaron M.; Kirkpatrick, J. Davy; Schneider, Adam C. +15 more

In an effort to identify nearby and unusual cold objects in the solar neighborhood, we searched for previously unidentified moving objects using CatWISE2020 proper motion data combined with machine learning methods. We paired the motion candidates with their counterparts in 2MASS, UHS, and VHS. Then we searched for white dwarf, brown dwarf, and su…

2022 The Astronomical Journal
Gaia 10
Independent Evidence for Earlier Formation Epochs of Fossil Groups of Galaxies through the Intracluster Light: The Case for RX J100742.53+380046.6
DOI: 10.3847/1538-4357/ac7f3f Bibcode: 2022ApJ...936...59D

Koekemoer, Anton M.; Dupke, Renato A.; Carrasco, Eleazar R. +9 more

Fossil groups (FG) of galaxies still present a puzzle to theories of structure formation. Despite the low number of bright galaxies, they have relatively high velocity dispersions and ICM temperatures often corresponding to cluster-like potential wells. Their measured concentrations are typically high, indicating early formation epochs as expected…

2022 The Astrophysical Journal
XMM-Newton eHST 10