Search Publications

Reconstructing the genesis of a globular cluster system at a look-back time of 9.1 Gyr with the JWST
DOI: 10.1093/mnrasl/slac162 Bibcode: 2023MNRAS.520L..58F

Forbes, Duncan A.; Romanowsky, Aaron J.

Using early-release data from the JWST, Mowla et al. and Claeyssens et al. recently measured various properties for gravitationally lensed compact sources ('sparkles') around the 'Sparkler' galaxy at a redshift of 1.378 (a look-back time of 9.1 Gyr). Here, we focus on the Mowla et al. as they were able to break the age-metallicity degeneracy and d…

2023 Monthly Notices of the Royal Astronomical Society
JWST 8
Strong and Rapid X-Ray Variability of the Super-Eddington Accreting Quasar SDSS J081456.10+532533.5
DOI: 10.3847/1538-4357/accd64 Bibcode: 2023ApJ...950...18H

Brandt, W. N.; Garmire, Gordon P.; Luo, Bin +6 more

We report strong and rapid X-ray variability found from the super-Eddington accreting quasar SDSS J081456.10+532533.5 at z = 0.1197. It has a black hole mass of 2.7 × 107 M and a dimensionless accretion rate of ≈4 measured from reverberation-mapping observations. It showed weak X-ray emission in the 2021 February Chandra ob…

2023 The Astrophysical Journal
XMM-Newton 8
Denoising Diffusion Probabilistic Models to Predict the Density of Molecular Clouds
DOI: 10.3847/1538-4357/accae5 Bibcode: 2023ApJ...950..146X

Xu, Duo; Tan, Jonathan C.; Hsu, Chia-Jung +1 more

We introduce the state-of-the-art deep-learning denoising diffusion probabilistic model as a method to infer the volume or number density of giant molecular clouds (GMCs) from projected mass surface density maps. We adopt magnetohydrodynamic simulations with different global magnetic field strengths and large-scale dynamics, i.e., noncolliding and…

2023 The Astrophysical Journal
Herschel 8
Time series analysis of bright TESS RRc stars: additional modes, phase variations, and more
DOI: 10.1093/mnras/stad556 Bibcode: 2023MNRAS.521..443B

Pál, A.; Plachy, E.; Molnár, L. +3 more

Using two years of data from the TESS space telescope, we have investigated the time series of 633 overtone pulsating field RR Lyrae (RRc) stars. The majority of stars (82.8 per cent) contain additional frequencies beyond the main pulsation. In addition to the frequencies previously explained by the ℓ = 8 and 9 non-radial modes, we have identified…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 8
Photometric Calibrations of M-dwarf Metallicity with Markov Chain Monte Carlo and Bayesian Inference
DOI: 10.3847/1538-4357/acacf6 Bibcode: 2023ApJ...944..106D

Caballero, J. A.; Montes, D.; Duque-Arribas, C. +3 more

Knowledge of stellar atmospheric parameters (T eff, $\mathrm{log}g$ , [Fe/H]) of M dwarfs can be used to constrain both theoretical stellar models and Galactic chemical evolutionary models, and guide exoplanet searches, but their determination is difficult due to the complexity of the spectra of their cool atmospheres. In our ongoing ef…

2023 The Astrophysical Journal
Gaia 8
X-ray and optical spectroscopic study of a γ Cassiopeiae analog source π Aquarii
DOI: 10.1093/pasj/psac099 Bibcode: 2023PASJ...75..177T

Tsujimoto, Masahiro; Hayashi, Takayuki; Morihana, Kumiko +1 more

γ Cas analog sources are a subset of Be stars that emit intense and hard X-ray emission. Two competing ideas for their X-ray production mechanism are (a) the magnetic activities of the Be star and its disk and (b) the accretion from the Be star to an unidentified compact object. Among such sources, π Aqr plays a pivotal role as it is one of the on…

2023 Publications of the Astronomical Society of Japan
Gaia XMM-Newton 8
The X-Ray Binary-star Cluster Connection in Late-type Galaxies
DOI: 10.3847/1538-4357/ace162 Bibcode: 2023ApJ...953..126H

Chandar, Rupali; Maccarone, Thomas J.; Thilker, David A. +3 more

We conduct one of the largest systematic investigations of bright X-ray binaries (XRBs) in both young star clusters and ancient globular clusters (GCs) using a sample of six nearby star-forming galaxies. Combining complete CXO X-ray source catalogs with optical Physics at High Angular Resolution in Nearby Galaxies-Hubble Space Telescope cluster ca…

2023 The Astrophysical Journal
eHST 8
Non-thermal Broadening of IRIS Fe XXI Line Caused by Turbulent Plasma Flows in the Magnetic Reconnection Region During Solar Eruptions
DOI: 10.3389/fspas.2023.1096133 Bibcode: 2023FrASS..1096133S

Reeves, Katharine K.; Polito, Vanessa; Chen, Bin +3 more

Magnetic reconnection is the key mechanism for energy release in solar eruptions, where the high-temperature emission is the primary diagnostic for investigating the plasma properties during the reconnection process. Non-thermal broadening of high-temperature lines has been observed in both the reconnection current sheet (CS) and flare loop-top re…

2023 Frontiers in Astronomy and Space Sciences
Hinode IRIS 8
Star-forming site RAFGL 5085: Is a perfect candidate of hub-filament system?
DOI: 10.1007/s12036-022-09907-7 Bibcode: 2023JApA...44...23D

Dewangan, L. K.; Pandey, Rakesh; Sharma, Saurabh +4 more

To investigate the star-formation process, we present a multi-wavelength study of a massive star-forming site RAFGL 5085, which has been associated with the molecular outflow, HII region and near-infrared cluster. The continuum images at 12, 250, 350 and 500 µm …

2023 Journal of Astrophysics and Astronomy
Gaia Herschel 8
Environmental Impacts on the Rest-frame UV Size and Morphology of Star-forming Galaxies at z 2
DOI: 10.3847/1538-4357/acfb81 Bibcode: 2023ApJ...958..170N

Koyama, Yusei; Kodama, Tadayuki; Shimakawa, Rhythm +1 more

We report the measurement of rest-frame UV size and morphology of Hα-emission-selected star-forming galaxies (HAEs) in four protoclusters at z ~ 2 (PKS 1138-262, USS 1558-003, PHz G237.0+42.5, and CC 2.2) using archival Hubble Space Telescope Advanced Camera Survey (HST/ACS) F814W data. We compare the measurement of 122 HAEs in protoclusters detec…

2023 The Astrophysical Journal
eHST 8