Search Publications

Detailed asteroseismic modelling of RR Lyrae stars with non-radial modes
DOI: 10.1093/mnras/stad2611 Bibcode: 2023MNRAS.525.5378N

Molnár, L.; Netzel, H.; Joyce, M.

Photometric observations from the last decade have revealed additional low-amplitude periodicities in many classical pulsators that are likely due to pulsations in non-radial modes. One group of multimode RR Lyrae stars, the so-called 0.61 stars, is particularly interesting. In these stars, the radial first overtone is accompanied by additional si…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 7
Cold mode gas accretion on two galaxy groups at z ∼ 2
DOI: 10.1093/mnras/stac3537 Bibcode: 2023MNRAS.519..961V

Zakamska, Nadia L.; Armus, Lee; Wright, Shelley A. +5 more

We present Keck Cosmic Web Imager (KCWI) integral field spectroscopy (IFS) observations of rest-frame UV emission lines $\rm Ly\alpha$, CIVλλ 1548 Å, 1550Å, and $\rm HeII$ 1640 Å observed in the circumgalactic medium (CGM) of two z = 2 radio-loud quasar host galaxies. We detect extended emission on 80-90 kpc scale in $\rm Ly\alpha$ in both systems…

2023 Monthly Notices of the Royal Astronomical Society
eHST 7
Solar Coronal Density Turbulence and Magnetic Field Strength at the Source Regions of Two Successive Metric Type II Radio Bursts
DOI: 10.3847/1538-4357/acaea5 Bibcode: 2023ApJ...943...43R

Kumari, Anshu; Ramesh, R.; Kathiravan, C.

We report spectral and polarimeter observations of two weak, low-frequency (≈85-60 MHz) solar coronal type II radio bursts that occurred on 2020 May 29 within a time interval ≈2 minutes. The bursts had fine structures, and were due to harmonic plasma emission. Our analysis indicates that the magnetohydrodynamic shocks responsible for the first and…

2023 The Astrophysical Journal
SOHO 7
Spectroscopically Identified Cataclysmic Variables from the LAMOST Survey. II. Period Estimates
DOI: 10.3847/1538-3881/aca906 Bibcode: 2023AJ....165..148H

Luo, A. -Li; Hou, Wen; Bai, Zhong-Rui +2 more

We examine a sample of 340 cataclysmic variables (CVs) from the latest data release of the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) survey, along with 18 objects that are newly classified as CVs. In this paper, we focus on investigating the photometric behaviors of these CVs using data from time-domain surveys. The orbita…

2023 The Astronomical Journal
Gaia 7
CO Survey of High-z Radio Galaxies, Revisited with the Atacama Large Millimeter/submillimeter Array: Jet-Cloud Alignments and Synchrotron Brightening by Molecular Gas in the Circumgalactic Environment
DOI: 10.3847/1538-4357/acde53 Bibcode: 2023ApJ...952..148E

Carilli, Chris; Lehnert, Matthew D.; De Breuck, Carlos +6 more

Powerful radio sources associated with supermassive black holes are among the most luminous objects in the universe, and are frequently recognized both as cosmological probes and active constituents in the evolution of galaxies. We present alignments between radio jets and cold molecular gas in the environment of distant radio galaxies, and show t…

2023 The Astrophysical Journal
eHST 7
Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si - III. Grids of isochrones for -2.5 ≤ [Fe/H] ≤ -0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity
DOI: 10.1093/mnras/stac3270 Bibcode: 2023MNRAS.518.4517V

VandenBerg, Don A.

Stellar evolutionary tracks for $0.12 \le {\cal M}/{\cal M_{\odot }}\le 1.0$ have been computed for each of several variations in the abundances of C, N, and O, assuming mass-fraction helium abundances Y = 0.25 and 0.29, and 11 metallicities in the range -2.5 ≤ [Fe/H] ≤ -0.5, in 0.2-dex increments. Such computations are provided for mixtures with …

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 7
The impact of black hole scaling relation assumptions on the mass density of black holes
DOI: 10.1093/mnras/stad2146 Bibcode: 2023MNRAS.524.4403M

Simon, Joseph; Gültekin, Kayhan; Matt, Cayenne

We examine the effect of supermassive black hole (SMBH) mass scaling relation choice on the inferred SMBH mass population since redshift z ~ 3. To make robust predictions for the gravitational wave background (GWB), we must have a solid understanding of the underlying SMBH demographics. Using the SDSS and 3D-HST + CANDELS surveys for 0 < z <…

2023 Monthly Notices of the Royal Astronomical Society
eHST 7
Periodic X-ray sources in the massive globular cluster 47 Tucanae: Evidence for dynamically formed cataclysmic variables
DOI: 10.1093/mnras/stad836 Bibcode: 2023MNRAS.521.4257B

Li, Zhiyuan; Bao, Tong; Cheng, Zhongqun

We present a systematic study of periodic X-ray sources in the massive globular cluster 47 Tuc, utilizing deep archival Chandra observations that resolve the cluster core and recently available eROSITA observations that cover the cluster outskirt. By applying the Gregory-Loredo algorithm, we detect 20 periodic signals among 18 X-ray sources, rangi…

2023 Monthly Notices of the Royal Astronomical Society
eHST 7
Large-scale Spatial Cross-calibration of Hinode/SOT-SP and SDO/HMI
DOI: 10.3847/1538-4365/aca539 Bibcode: 2023ApJS..264...49F

Liu, Yang; Antiochos, Spiro K.; Leka, K. D. +7 more

We investigate the cross-calibration of the Hinode/Solar Optical Telescope-Spectro-Polarimeter (SOT-SP) and Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI) instrument metadata, specifically the correspondence of the scaling and pointing information. Accurate calibration of these data sets gives the correspondence needed by in…

2023 The Astrophysical Journal Supplement Series
Hinode 7
Carbon Dioxide Retrievals From NOMAD-SO on ESA's ExoMars Trace Gas Orbiter and Temperature Profile Retrievals With the Hydrostatic Equilibrium Equation: 2. Temperature Variabilities in the Mesosphere at Mars Terminator
DOI: 10.1029/2022JE007279 Bibcode: 2023JGRE..12807279T

Aoki, S.; Vandaele, A. C.; Daerden, F. +14 more

The Solar Occultation (SO) channel of the Nadir and Occultation for Mars Discovery (NOMAD) instrument scans the Martian atmosphere since 21 April 2018. In this work, we present a subset of the NOMAD SO data measured at the mesosphere. We focused on a spectral range that started to be recorded in Martian year (MY) 35. A total of 968 vertical profil…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 7