Search Publications

Mass Function of a Young Cluster in a Low-metallicity Environment. Sh 2-209
DOI: 10.3847/1538-4357/ac94d5 Bibcode: 2023ApJ...943..137Y

Kobayashi, Naoto; Izumi, Natsuko; Saito, Masao +2 more

We present deep near-infrared (NIR) imaging of Sh 2-209 (S209), a low-metallicity ([O/H] = -0.5 dex) H II region in the Galaxy. From the NIR images, combined with astrometric data from Gaia EDR3, we estimate the distance to S209 to be 2.5 kpc. This is close enough to enable us to resolve cluster members clearly (≃1000 au separation) down to a mass…

2023 The Astrophysical Journal
Gaia 9
Investigating Pre-eruptive Magnetic Properties at the Footprints of Erupting Magnetic Flux Ropes
DOI: 10.3847/1538-4357/aca6e1 Bibcode: 2023ApJ...943...80W

Qiu, Jiong; Wang, Yuming; Liu, Rui +4 more

It is well established that solar eruptions are powered by free magnetic energy stored in the current-carrying magnetic field in the corona. It has also been generally accepted that magnetic flux ropes (MFRs) are a critical component of many coronal mass ejections. What remains controversial is whether MFRs are present well before the eruption. Ou…

2023 The Astrophysical Journal
SOHO 9
Stars, Gas, and Star Formation of Distant Post-starburst Galaxies
DOI: 10.3847/1538-4357/acf0bd Bibcode: 2023ApJ...955...75W

Maseda, Michael V.; D'Eugenio, Francesco; van der Wel, Arjen +5 more

We present a comprehensive multiwavelength study of five post-starburst galaxies with M * > 1011 M at z ~ 0.7, examining their stars, gas, and current and past star formation activities. Using optical images from the Subaru Telescope and Hubble Space Telescope, we observe a high incidence of companion galaxies…

2023 The Astrophysical Journal
eHST 9
Chromospheric Heating from Local Magnetic Growth and Ambipolar Diffusion under Nonequilibrium Conditions
DOI: 10.3847/2041-8213/acafe9 Bibcode: 2023ApJ...943L..14M

Martínez-Sykora, Juan; De Pontieu, Bart; Hansteen, Viggo H. +3 more

The heating of the chromosphere in internetwork regions remains one of the foremost open questions in solar physics. In the present study, we tackle this old problem by using a very-high-spatial-resolution simulation of quiet-Sun conditions performed with radiative MHD numerical models and interface region imaging spectrograph (IRIS) observations.…

2023 The Astrophysical Journal
IRIS 9
Interpreting the Si II and C II Line Spectra from the COS Legacy Archive Spectroscopic SurveY Using a Virtual Galaxy from a High-resolution Radiation-hydrodynamic Simulation
DOI: 10.3847/1538-4357/acda2c Bibcode: 2023ApJ...952..164G

Wilkins, Stephen M.; Martin, Crystal L.; Garel, Thibault +19 more

Observations of low-ionization state metal lines provide crucial insights into the interstellar medium (ISM) of galaxies, yet, disentangling the physical processes responsible for the emerging line profiles is difficult. This work investigates how mock spectra generated using a single galaxy in a radiation-hydrodynamical simulation can help us int…

2023 The Astrophysical Journal
eHST 9
Internal Kinematics and Structure of the Bulge Globular Cluster NGC 6569
DOI: 10.3847/1538-4357/accce9 Bibcode: 2023ApJ...950..138P

Vesperini, Enrico; Cadelano, Mario; Pallanca, Cristina +8 more

In the context of a project aimed at characterizing the properties of star clusters in the Galactic bulge, here we present the determination of the internal kinematics and structure of the massive globular cluster NGC 6569. The kinematics has been studied by means of an unprecedented spectroscopic data set acquired in the context of the ESO-VLT Mu…

2023 The Astrophysical Journal
Gaia eHST 9
Extinction of Taurus, Orion, Perseus, and California Molecular Clouds Based on the LAMOST, 2MASS, and Gaia Surveys. I. 3D Extinction and Structure
DOI: 10.3847/1538-4357/acbbc7 Bibcode: 2023ApJ...945..132C

Jiang, Biwei; Zhao, He; Sun, Mingxu +1 more

The 3D extinction and structure are studied for the Taurus, Orion, Perseus, and California molecular clouds based on the LAMOST spectroscopy. Stellar color excess is calculated with the intrinsic color index derived from the atmospheric parameters in the LAMOST DR8 catalog and the observed color index in the Gaia EDR3 and the 2MASS PSC. In combina…

2023 The Astrophysical Journal
Gaia 9
Observational Signatures of Electron-driven Chromospheric Evaporation in a White-light Flare
DOI: 10.3847/1538-4357/ace256 Bibcode: 2023ApJ...954....7L

Warmuth, Alexander; Li, Dong; Ning, Zongjun +7 more

We investigate observational signatures of explosive chromospheric evaporation during a white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis, bisector techniques, and the Gaussian fitting method, redshifted velocities of less than 20 km s‑1 are detected in low-temperature spectral lines of Hα, C I, and Si I…

2023 The Astrophysical Journal
IRIS SolarOrbiter 9
Dust-buried Compact Sources in the Dwarf Galaxy NGC 4449
DOI: 10.3847/1538-4357/acbeac Bibcode: 2023ApJ...946....1C

Ji, Zhiyuan; Smith, Linda J.; Calzetti, Daniela +10 more

Multiwavelength images from the Hubble Space Telescope covering the wavelength range 0.27-1.6 µm show that the central area of the nearby dwarf galaxy NGC 4449 contains several tens of compact sources that are emitting in the hydrogen recombination line Paβ (1.2818 µm) but are only marginally detected in Hα (0.6563 µm) and undete…

2023 The Astrophysical Journal
eHST 9
Serendipitous Nebular-phase JWST Imaging of SN Ia SN 2021aefx: Testing the Confinement of 56Co Decay Energy
DOI: 10.3847/2041-8213/acb6d8 Bibcode: 2023ApJ...944L..28C

Galbany, L.; Morrell, Nidia; Leroy, Adam K. +29 more

We present new 0.3-21 µm photometry of SN 2021aefx in the spiral galaxy NGC 1566 at +357 days after B-band maximum, including the first detection of any Type Ia supernova (SN Ia) at >15 µm. These observations follow earlier JWST observations of SN 2021aefx at +255 days after the time of maximum brightness, allowing us to probe the t…

2023 The Astrophysical Journal
JWST 9