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A Novel Survey for Young Substellar Objects with the W-band Filter. V. IC 348 and Barnard 5 in the Perseus Cloud
DOI: 10.3847/1538-3881/ac8547 Bibcode: 2022AJ....164..125L

Jose, Jessy; Allers, Katelyn; Albert, Loïc +10 more

We report the discovery of substellar objects in the young star cluster IC 348 and the neighboring Barnard 5 dark cloud, both at the eastern end of the Perseus star-forming complex. The substellar candidates are selected using narrowband imaging, i.e., on and off photometric technique with a filter centered around the water absorption feature at 1…

2022 The Astronomical Journal
Gaia 7
AstroSat/UVIT Cluster Photometry in the Northern Disk of M31
DOI: 10.3847/1538-3881/ac9058 Bibcode: 2022AJ....164..183L

Leahy, Denis; Buick, Megan; Leahy, Cameron

The Andromeda galaxy (M31) is an object of ongoing study with the Ultraviolet Imaging Telescope (UVIT) on AstroSat. UVIT far-UV (FUV) and near-UV (NUV) photometry is carried out here for a set of 239 clusters in the NE disk and bulge of M31 that overlap with the HST/PHAT survey. Padova stellar models were applied to derive ages, masses, metallicit…

2022 The Astronomical Journal
eHST 7
Living on the edge of the Milky Way's central molecular zone. G1.3 is the more likely candidate for gas accretion into the CMZ
DOI: 10.1051/0004-6361/202244870 Bibcode: 2022A&A...668A.183B

Menten, Karl M.; Kauffmann, Jens; Güsten, Rolf +3 more

Context. The 1°.3 (G1.3) and 1°.6 (G1.6) cloud complexes in the central molecular zone (CMZ) of our Galaxy have been proposed to possibly reside at the intersection region of the X1 and X2 orbits for several reasons. This includes the detection of co-spatial low- and high-velocity clouds, high velocity dispersion, high fractional molecular abundan…

2022 Astronomy and Astrophysics
Herschel 7
A detailed study of the bridge of excess X-ray emission between the galaxy clusters Abell 2029 and Abell 2033
DOI: 10.1093/mnras/stab2979 Bibcode: 2022MNRAS.509.1109M

Walker, S. A.; Mirakhor, M. S.; Runge, J.

We examine Suzaku, XMM-Newton, and Chandra observations of the Abell 2029/2033 system to investigate the nature of a bridge of X-ray emission joining the two galaxy clusters. By modelling the contributions from the outskirts of the two clusters, and excluding the emission from the southern infalling group and the background group LOS9, we find a s…

2022 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 7
Solar Polar Magnetic Fields: Comparing Full-disk and High-resolution Spectromagnetograph Data
DOI: 10.3847/1538-4357/aca1a8 Bibcode: 2022ApJ...941..142P

Petrie, Gordon J. D.

This is the first systematic comparison between photospheric polar magnetic field data from a full-disk synoptic observing program, the National Solar Observatory's Synoptic Optical Long-term Investigations of the Sun Vector Spectromagnetograph (SOLIS/VSM), and a high-resolution vector spectromagnetograph, the Hinode Solar Optical Telescope Spectr…

2022 The Astrophysical Journal
Hinode 7
Electron Diffusion by Magnetosonic Waves in the Earth's Radiation Belts
DOI: 10.1029/2021JA030196 Bibcode: 2022JGRA..12730196W

Meredith, Nigel P.; Wong, Jin-Mann; Horne, Richard B. +2 more

We conduct a global survey of magnetosonic waves and compute the associated bounce- and drift-averaged diffusion coefficients, taking into account colocated measurements of fpe/fce, to assess the role of magnetosonic waves in radiation belt dynamics. The average magnetosonic wave intensities increase with increasing geomagnet…

2022 Journal of Geophysical Research (Space Physics)
Cluster 7
Catching a grown-up starfish planetary nebula - II. Plasma analysis and central star properties of PC 22
DOI: 10.1093/mnras/stab3649 Bibcode: 2022MNRAS.511....1S

Morisset, C.; Guerrero, M. A.; Todt, H. +4 more

After performing the morpho-kinematic analysis of the planetary nebula (PN) PC 22, we now present its nebular and stellar analysis. The plasma investigation relies on the novel use of a Monte Carlo analysis associated with the PYNEB code for the uncertainty propagation. The innermost region of the nebula shows electronic temperatures Te

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Rate of Change of Large-Scale Solar-Wind Structure
DOI: 10.1007/s11207-022-02006-4 Bibcode: 2022SoPh..297...83O

Riley, Pete; Lockwood, Mike; Owens, Mathew J. +5 more

Quantifying the rate at which the large-scale solar-wind structure evolves is important for both understanding the physical processes occurring in the corona and for space-weather forecast improvement. Models of the global corona and heliosphere typically assume that the ambient solar-wind structure is steady and corotates with the Sun, which is g…

2022 Solar Physics
SOHO 7
Constraining the formation of paleolake inlet valleys across crater rims
DOI: 10.1016/j.icarus.2022.114945 Bibcode: 2022Icar..37814945B

Goudge, Timothy A.; Fassett, Caleb I.; Osinski, Gordon R. +1 more

Impact crater lakes with an inlet valley were common on Mars during past epochs. However, it has not been established exactly how impact craters with initially high-standing rims were breached by an inlet. We investigated four potential mechanisms for inlet valley breach formation: (1) rim erosion, (2) depositional rim burial, (3) drainage head er…

2022 Icarus
MEx 7
Predicting the Geoeffectiveness of CMEs Using Machine Learning
DOI: 10.3847/1538-4357/ac7962 Bibcode: 2022ApJ...934..176P

Besliu-Ionescu, Diana; Paraschiv, Alin Razvan; Pricopi, Andreea-Clara +1 more

Coronal mass ejections (CMEs) are the most geoeffective space weather phenomena, being associated with large geomagnetic storms, and having the potential to cause disturbances to telecommunications, satellite network disruptions, and power grid damage and failures. Thus, considering these storms' potential effects on human activities, accurate for…

2022 The Astrophysical Journal
SOHO 7