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The binary fraction of red supergiants in the Magellanic Clouds
Min Dai and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1220–1235, https://doi.org/10.1093/mnras/staf560
Red supergiants (RSGs), as the descendants of OB-type stars and the progenitors of supernovae, provide crucial insights into the evolution of massive stars, particularly in binary systems. Previous studies show that the binary fraction of RSGs ( $\approx 15\!-\!40~{{\ \rm per\ cent}}$ ) is ...
Field-level inference of H0 from simulated type Ia supernovae in a local Universe analogue
Eleni Tsaprazi and Alan F Heavens
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1448–1457, https://doi.org/10.1093/mnras/staf619
Two particular challenges face type Ia supernovae (SNeIa) as probes of the expansion rate of the Universe. One is that they may not be fair tracers of the matter velocity field and the second is that their peculiar velocities distort the Hubble expansion. Although the latter has been estimated at ...
Energy-resolved polarization study of the Crab nebula with IXPE
Wenhao Wei and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 902–909, https://doi.org/10.1093/mnras/staf538
This work presents a new detailed study on the energy-dependent variation in the X-ray polarization of the Crab pulsar wind nebula (PWN), obtained using data from the Imaging X-ray Polarimetry Explorer ( IXPE ). For the entire PWN, we observed a linear variation in polarization degree (PD), and ...
Life in the slow lane: a search for long-term variability in ASAS-SN
Sydney Petz and C S Kochanek
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1065–1076, https://doi.org/10.1093/mnras/staf587
We search a sample of 9361 613 isolated sources with 13< g <14.5 mag for slowly varying sources. We select sources with brightness changes larger than $\sim 0.03$ mag yr −1 over 10 yr, removing false positives due to, for example, nearby bright stars or high proper motions. After a thorough ...
Exploring the fate of primordial discs in Milky Way-sized galaxies with the GigaEris simulation
Floor van Donkelaar and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1259–1268, https://doi.org/10.1093/mnras/staf597
Recent observations with JWST and Atacama Large Millimeter/submillimeter Array (ALMA) have unveiled galaxies with regular discs at significantly higher redshifts than previously expected. This appears to be in contrast to our understanding of galaxy evolution at high redshift. Additionally, the ...
Numerical modelling of the lobes of radio galaxies – VI. Polarimetric simulations of universal pressure profile cluster atmospheres
M Stimpson and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1668–1691, https://doi.org/10.1093/mnras/staf610
We present the results of a polarization study based upon relativistic magnetohydrodynamic modelling of jets running into hydrostatic, spherically symmetric cluster atmospheres. For the first time in a numerical simulation, we derive Faraday rotation measure maps (RM maps) from model cluster ...
Deep Extragalactic VIsible Legacy Survey (DEVILS): new robust merger rates at intermediate redshifts
Melissa F Fuentealba-Fuentes and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1651–1667, https://doi.org/10.1093/mnras/staf596
Mergers are fundamental to our understanding of the processes driving the evolution of the structure and morphology of galaxies, star formation, active galactic nucleus activity, and the redistribution of stellar mass in the Universe. Determining the fraction and properties of mergers across cosmic ...
Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
Youcai Zhang and others
Monthly Notices of the Royal Astronomical Society, Volume 539, Issue 2, May 2025, Pages 1692–1705, https://doi.org/10.1093/mnras/staf611
Using galaxies from the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) along with haloes from the dark matter only constrained ELUCID (Exploring the Local Universe with the reConstructed Initial Density field) simulation, we examine the properties of galaxies and haloes with respect to their ...

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