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New, late-type spectroscopic binaries with X-ray emission
DOI: 10.1093/mnras/stac1850 Bibcode: 2022MNRAS.515.3716F

Guillout, P.; Giarrusso, M.; Leone, F. +6 more

In this paper, we present a spectroscopic study of six double-lined binaries, five of which were recently discovered in a high-resolution spectroscopic survey of optical counterparts of stellar X-ray sources. Thanks to high-resolution spectra acquired with CAOS spectropolarimeter during 7 yr, we were able to measure the radial velocities of their …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Searching for Diamagnetic Blob Accretion in the 74 day K2 Observation of V2400 Ophiuchi
DOI: 10.3847/1538-3881/ac3010 Bibcode: 2022AJ....163....4L

Garnavich, Peter; Littlefield, Colin; Szkody, Paula +3 more

Since its discovery in 1995, V2400 Ophiuchi (V2400 Oph) has stood apart from most known intermediate polar cataclysmic variables due to its proposed magnetic field strength (9-27 MG) and diskless accretion. To date, the exact accretion mechanism of the system is still unknown, and standard accretion models fail to accurately predict the peculiar b…

2022 The Astronomical Journal
Gaia 2
Constraining Mass of M31 Combing Kinematics of Stars, Planetary Nebulae and Globular clusters
DOI: 10.1088/1674-4527/ac7af9 Bibcode: 2022RAA....22h5023Y

Fan, Zhou; Zhu, Ling; Liu, Cheng +2 more

We construct a multiple-population discrete axisymmetric Jeans model for the Andromeda (M31) galaxy, considering three populations of kinematic tracers: 48 supergiants and 721 planetary nebulae (PNe) in the bulge and disk regions, 554 globular clusters extending to ~30 kpc, and halo stars extending to ~150 kpc of the galaxy. The three populations …

2022 Research in Astronomy and Astrophysics
Gaia 2
Strong Spatial Aggregation of Martian Surface Temperature Shaped by Spatial and Seasonal Variations in Meteorological and Environmental Factors
DOI: 10.1088/1674-4527/ac3896 Bibcode: 2022RAA....22a5015L

Li, Fei; Barriot, Jean-Pierre; Luo, Yao-Wen +1 more

Spatio-temporal variation in the Martian surface temperature (MST) is an indicator of ground level thermal processes and hence a building block for climate models. However, the distribution of MST exhibits different levels of spatial aggregation or heterogeneity, and varies in space and time. Furthermore, the effect of regional differences in mete…

2022 Research in Astronomy and Astrophysics
MEx 2
Generation and Optimization of Spectral Cluster Maps to Enable Data Fusion of CaSSIS and CRISM Datasets
DOI: 10.3390/rs14112524 Bibcode: 2022RemS...14.2524F

Thomas, Nicolas; Rossi, Angelo Pio; Fernandes, Michael +2 more

Four-band color imaging of the Martian surface using the Color and Stereo Surface Imaging System (CaSSIS) onboard the European Space Agency's ExoMars Trace Gas Orbiter exhibits a high color diversity in specific regions. Not only is the correlation of color diversity maps with local morphological properties desirable, but mineralogical interpretat…

2022 Remote Sensing
ExoMars-16 2
Venus mountain waves in the upper atmosphere simulated by a time-invariant linear full-wave spectral model
DOI: 10.1016/j.icarus.2022.114922 Bibcode: 2022Icar..37714922H

Schubert, Gerald; Navarro, Thomas; Walterscheid, Richard L. +1 more

A 2-D spectral full-wave model is described that simulates the generation and propagation of mountain waves over idealized topography in Venus' atmosphere. Modeled temperature perturbations are compared with the Akatsuki observations. Lower atmosphere eddy diffusivity and stability play a major role in the upward propagation of gravity waves from …

2022 Icarus
VenusExpress 2
A census of young stellar objects in two line-of-sight star-forming regions toward IRAS 22147+5948 in the outer Galaxy
DOI: 10.1051/0004-6361/202141676 Bibcode: 2022A&A...663A.133K

Szczerba, Ryszard; Elia, Davide; Fischer, William J. +9 more

Context. Star formation in the outer Galaxy, namely, outside of the Solar circle, has not been extensively studied in part due to the low CO brightness of the molecular clouds linked with the negative metallicity gradient. Recent infrared surveys provide an overview of dust emission in large sections of the Galaxy, but they suffer from cloud confu…

2022 Astronomy and Astrophysics
Gaia Herschel 2
Identifying Shadowing Signatures of C Ring Ringlets and Plateaus in Cassini Data from Saturn's Ionosphere
DOI: 10.3847/PSJ/ac7790 Bibcode: 2022PSJ.....3..168D

Vigren, Erik; Wahlund, Jan-Erik; Dreyer, Joshua +5 more

For orbits 288 and 292 of Cassini's Grand Finale, clear dips (sharp and narrow decreases) are visible in the ${{\rm{H}}}_{2}^{+}$ densities measured by the Ion and Neutral Mass Spectrometer (INMS). In 2017, the southern hemisphere of Saturn was shadowed by its rings and the substructures within. Tracing a path of the solar photons through the ring…

2022 The Planetary Science Journal
Cassini 2
A GMOS/IFU Study of Jellyfish Galaxies in Massive Clusters
DOI: 10.3847/1538-4357/ac9276 Bibcode: 2022ApJ...940...24L

Lee, Myung Gyoon; Lee, Jeong Hwan; Kang, Jisu +2 more

Jellyfish galaxies are an intriguing snapshot of galaxies undergoing ram pressure stripping (RPS) in dense environments, showing spectacular star-forming knots in their disks and tails. We study the ionized gas properties of five jellyfish galaxies in massive clusters with Gemini GMOS/Integral Field Unit observations: MACSJ0916-JFG1 (z = 0.330), M…

2022 The Astrophysical Journal
eHST 2
Generation of Large-Scale Orthophoto Mosaics Using MEX HRSC Images for the Candidate Landing Regions of China's First Mars Mission
DOI: 10.1109/TGRS.2021.3128518 Bibcode: 2022ITGRS..6028518G

Geng, Xun; Xu, Qing; Wang, Jiayao +3 more

2022 IEEE Transactions on Geoscience and Remote Sensing
MEx 2