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Solar Wind Charge Exchange Soft X-Ray Emissions in the Magnetosphere during an Interplanetary Coronal Mass Ejection Compared to Its Driven Sheath
DOI: 10.3847/2041-8213/ac7521 Bibcode: 2022ApJ...932L...1Z

Liu, Ying D.; Sun, Wei; Ji, Li +9 more

Soft X-ray emissions from solar wind charge exchange (SWCX) are applied in a recently developed approach to study the magnetosphere using panoramic soft X-ray imaging. This study represents the first attempt to distinguish magnetospheric SWCX emissions observed by XMM-Newton during the impact of an interplanetary coronal mass ejection (ICME) and i…

2022 The Astrophysical Journal
XMM-Newton 11
An Electric-field-driven Global Coronal Magnetohydrodynamics Simulation Model Using Helioseismic and Magnetic Imager Vector-magnetic-field Synoptic Map Data
DOI: 10.3847/1538-4357/ac6173 Bibcode: 2022ApJ...930...60H

Hayashi, Keiji; Wu, Chin-Chun; Liou, Kan

We present the simulation methodology and results of our new data-driven global coronal magnetohydrodynamics (MHD) simulation model. In this model, the solar-surface electric field is first calculated such that the curl will satisfy both the induction equation and the given temporal variations of the solar-surface magnetic field. We use the synopt…

2022 The Astrophysical Journal
SOHO 11
New Theoretical Period-Luminosity-Metallicity Relations for RR Lyrae in the Rubin-LSST Filters
DOI: 10.3847/1538-4357/ac78ee Bibcode: 2022ApJ...934...29M

Marconi, Marcella; Molinaro, Roberto; Dall'Ora, Massimo +8 more

The revolutionary power of future Rubin-LSST observations will allow us to significantly improve the physics of pulsating stars, including RR Lyrae. In this context, an updated theoretical scenario predicting all the relevant pulsation observables in the corresponding photometric filters is mandatory. The bolometric light curves are based on a rec…

2022 The Astrophysical Journal
Gaia 11
The Extended Tidal Tails of NGC 7089 (M2)
DOI: 10.3847/1538-4357/ac5bd7 Bibcode: 2022ApJ...929...89G

Grillmair, Carl J.

Using photometry and proper motions from Gaia Early Data Release 3, we detect a 45° long trailing stellar debris stream associated with the old, metal-poor globular cluster NGC 7089. With a width on the order of 100 pc, the extended stream appears to be as dynamically cold as the coldest known streams found to date. There is some evidence for an e…

2022 The Astrophysical Journal
Gaia 11
Blue Stragglers as Tracers of the Dynamical State of Two Clusters in the Small Magellanic Cloud: NGC 339 and NGC 419
DOI: 10.3847/1538-4357/ac5406 Bibcode: 2022ApJ...928...47D

Dalessandro, E.; Massari, D.; Ferraro, F. R. +5 more

The level of central segregation of Blue Straggler stars has proved to be an excellent tracer of the dynamical evolution of old star clusters (the so-called "dynamical clock"), both in the Milky Way and in the Large Magellanic Cloud. The A + parameter, used to measure the Blue Stragglers degree of segregation, has in fact been found to …

2022 The Astrophysical Journal
eHST 11
Milky Way Zero-point Calibration of the JAGB Method: Using Thermally Pulsing AGB Stars in Galactic Open Clusters
DOI: 10.3847/1538-4357/ac92fd Bibcode: 2022ApJ...938..125M

Madore, Barry F.; Freedman, Wendy L.; Lee, Abigail J. +1 more

We present a new calibration of the J-band absolute magnitude of the JAGB method based on thermally pulsing AGB stars that are members of Milky Way open clusters, having distances and reddenings, independently compiled and published by Marigo. A total 17 of these photometrically selected J-Branch AGB stars give M J = -6.40 mag with a …

2022 The Astrophysical Journal
Gaia 11
Protostellar and Protoplanetary Disk Masses in the Serpens Region
DOI: 10.3847/1538-4357/ac8ff0 Bibcode: 2022ApJ...938...55A

Law, Charles J.; Williams, Jonathan P.; Ricci, Luca +4 more

We present the results from an Atacama Large Millimeter/submillimeter Array (ALMA) 1.3 mm continuum and 12CO (J = 2 - 1) line survey spread over 10 deg2 in the Serpens star-forming region of 320 young stellar objects, 302 of which are likely members of Serpens (16 Class I, 35 flat-spectrum, 235 Class II, and 16 Class III). Fr…

2022 The Astrophysical Journal
Gaia 11
60 Candidate High-velocity Stars Originating from the Sagittarius Dwarf Spheroidal Galaxy in Gaia EDR3
DOI: 10.3847/2041-8213/ac786d Bibcode: 2022ApJ...933L..13L

Shi, Jianrong; Ma, Jun; Du, Cuihua +3 more

Using proper motions from Gaia Early Data Release 3 (Gaia EDR3) and radial velocities from several surveys, we identify 60 candidate high-velocity stars with a total velocity greater than 75% of the escape velocity that probably originated from the Sagittarius dwarf spheroidal galaxy (Sgr) by orbital analysis. Sgr's gravity has little effect on th…

2022 The Astrophysical Journal
Gaia 11
GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion
DOI: 10.3847/1538-4357/ac8480 Bibcode: 2022ApJ...936...55B

Cochran, William D.; Endl, Michael; Mahadevan, Suvrath +31 more

We detail the follow-up and characterization of a transiting exo-Venus identified by TESS, GJ 3929b (TOI-2013b), and its nontransiting companion planet, GJ 3929c (TOI-2013c). GJ 3929b is an Earth-sized exoplanet in its star's Venus zone (P b = 2.616272 ± 0.000005 days; S b = ${17.3}_{-0.7}^{+0.8}$ S ) orbiting …

2022 The Astrophysical Journal
Gaia 11
On the Variation in the Volumetric Evolution of CMEs from the Inner to Outer Corona
DOI: 10.3847/1538-4357/ac5909 Bibcode: 2022ApJ...929...11M

Pant, Vaibhav; Patel, Ritesh; Majumdar, Satabdwa

Some of the major challenges faced in understanding the early evolution of coronal mass ejections (CMEs) are due to the limited observations in the inner corona (<3 R ) and the plane-of-sky measurements. In this work, we have thus extended the application of the Graduated Cylindrical Shell (GCS) model to inner coronal observations f…

2022 The Astrophysical Journal
SOHO 11