Search Publications

Determination of Sodium Abundance Ratio from Low-resolution Stellar Spectra and Its Applications
DOI: 10.3847/1538-4357/ac3423 Bibcode: 2022ApJ...925...35K

Koo, Jae-Rim; Beers, Timothy C.; Lee, Young Sun +2 more

We present a method to determine sodium abundance ratios ([Na/Fe]) using the Na I D doublet lines in low-resolution (R ~ 2000) stellar spectra. As stellar Na I D lines are blended with those produced by the interstellar medium, we developed a technique for removing the interstellar Na I D lines using the relationship between extinction, which is p…

2022 The Astrophysical Journal
Gaia 6
Contribution of Spicules to Solar Coronal Emission
DOI: 10.3847/1538-4357/ac879b Bibcode: 2022ApJ...937...71S

Klimchuk, James A.; Sarkar, Aveek; Sow Mondal, Shanwlee

Recent high-resolution imaging and spectroscopic observations have generated renewed interest in spicules' role in explaining the hot corona. Some studies suggest that some spicules, often classified as type II, may provide significant mass and energy to the corona. Here we use numerical simulations to investigate whether such spicules can produce…

2022 The Astrophysical Journal
Hinode 6
Kinematical Analysis of Substructure in the Southern Periphery of the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ac5621 Bibcode: 2022ApJ...928...95C

Monachesi, Antonela; Choi, Yumi; Majewski, Steven R. +10 more

We report the first 3D kinematical measurements of 88 stars in the direction of several recently discovered substructures in the southern periphery of the Large Magellanic Cloud (LMC) using a combination of Gaia proper motions and radial velocities from the APOGEE-2 survey. More specifically, we explore stars in assorted APOGEE-2 pointings in a re…

2022 The Astrophysical Journal
Gaia 6
Radiative Magnetohydrodynamic Simulation of the Confined Eruption of a Magnetic Flux Rope: Magnetic Structure and Plasma Thermodynamics
DOI: 10.3847/2041-8213/ac7c6f Bibcode: 2022ApJ...933L..29W

Ding, Mingde; Chen, Feng; Wang, Can +1 more

It is widely believed that magnetic flux ropes are the key structure of solar eruptions; however, their observable counterparts are not clear yet. We study a flare associated with flux rope eruption in a comprehensive radiative magnetohydrodynamic simulation of flare-productive active regions, especially focusing on the thermodynamic properties of…

2022 The Astrophysical Journal
Hinode 6
Could the Magnetic Star HD 135348 Possess a Rigidly Rotating Magnetosphere?
DOI: 10.3847/2041-8213/ac4333 Bibcode: 2022ApJ...924L..10J

Gagliano, Robert; Jayaraman, Rahul; Ricker, George R. +5 more

We report the detection and characterization of a new magnetospheric star, HD 135348, based on photometric and spectropolarimetric observations. The TESS light curve of this star exhibited variations consistent with stars known to possess rigidly rotating magnetospheres (RRMs), so we obtained spectropolarimetric observations using the Robert Stobi…

2022 The Astrophysical Journal
Gaia 6
Luminosity Function and Event Rate Density of XMM-Newton-selected Supernova Shock Breakout Candidates
DOI: 10.3847/1538-4357/ac5328 Bibcode: 2022ApJ...927..224S

Liu, Zhu; Yuan, Weimin; Sun, Hui +6 more

A dozen X-ray supernova shock breakout (SN SBO) candidates were reported recently based on XMM-Newton archival data, which increased the X-ray-selected SN SBO sample by an order of magnitude. Assuming that they are genuine SN SBOs, we study the luminosity function (LF) by improving on the method used in our previous work. The light curves and the …

2022 The Astrophysical Journal
XMM-Newton 6
Light from the Darkness: Detecting Ultra-diffuse Galaxies in the Perseus Cluster through Over-densities of Globular Clusters with a Log-Gaussian Cox Process
DOI: 10.3847/1538-4357/ac7b22 Bibcode: 2022ApJ...935....3L

van Dokkum, Pieter; Romanowsky, Aaron J.; Abraham, Roberto +6 more

We introduce a new method for detecting ultra-diffuse galaxies by searching for over-densities in intergalactic globular cluster populations. Our approach is based on an application of the log-Gaussian Cox process, which is a commonly used model in the spatial statistics literature but rarely used in astronomy. This method is applied to the globul…

2022 The Astrophysical Journal
eHST 6
The Solar Wind Parker Spiral Angle Distributions and Variations at 1 au
DOI: 10.3847/1538-4357/ac6bf3 Bibcode: 2022ApJ...931..105C

Xu, Qi; Xu, Xiaojun; Wang, Jing +8 more

Using the data from the Advanced Composition Explorer (ACE) and Wind spacecraft, we statistically studied the Parker spiral angle (PSA) of the solar wind magnetic field from 1998 to 2019 at 1 au. The PSA occurrences over both a Carrington rotation (CR) and a year can be well fitted by a Gaussian distribution. However, large-scale magnetic structur…

2022 The Astrophysical Journal
VenusExpress 6
Searching Extra-tidal Features around the Globular Cluster Whiting 1
DOI: 10.3847/1538-4357/ac6264 Bibcode: 2022ApJ...930...23N

Tian, Haijun; Tian, Hao; Carballo-Bello, Julio A. +14 more

Whiting 1 is a faint and young globular cluster in the halo of the Milky Way, and was suggested to have originated in the Sagittarius spherical dwarf galaxy (Sgr dSph). In this paper, we use the deep DESI Legacy Imaging Surveys to explore tentative spatial connection between Whiting 1 and the Sgr dSph. We redetermine the fundamental parameters of …

2022 The Astrophysical Journal
Gaia 6
The Astrometric Animation of Water Masers toward the Mira Variable BX Cam
DOI: 10.3847/1538-4357/ac9599 Bibcode: 2022ApJ...941..105X

Kim, Dong-Jin; Sun, Yan; Orosz, Gabor +20 more

We report very long baseline interferometry (VLBI) monitoring observations of the 22 GHz water (H2O) masers around the Mira variable BX Cam, which were carried out as a part of the EAVN Synthesis of Stellar Maser Animations project. Data of 37 epochs in total were obtained from 2018 May to 2021 June with a time interval of 3-4 weeks, sp…

2022 The Astrophysical Journal
Gaia 6