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@rasjournals.bsky.socialOct 15, 2026, 9:02 AM

Published in #MNRAS: "AGC 322753: A dark galaxy candidate detected by ALFALFA and FASHI", Monaci et al. This is Fig. 2: please visit academic.oup.com/mnras/advanc... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Colour image made by combining the g, r, and i filters from Legacy Surveys. The dashed circle represents the 3.5 arcmin beam of the Arecibo radio telescope, while the solid circle represents the 3 arcmin beam of FAST. The crosses indicate the beam centroids. The white square highlights the position of the claimed OC by C.-P. Zhang et al. (2024) for this FASHI source. The white hexagon highlights the background galaxy (SDSS J224559 + 335532). The intersection between the two beams is the most probable location for the OC of AGC 322753, highlighted in the red inset. Here, marked sources with the short horizontal and vertical lines are foreground stars confirmed with Gaia DR3, and the galaxy marked by a white arrow is in the background. See the text.
@rasjournals.bsky.socialOct 14, 2026, 8:15 AM

Published in #MNRAS: "Uncovering the origin of complex velocity distributions in edge-on disc galaxies", Townson et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Mock g-band image of Galaxy 102 viewed face-on (see M. Martig et al. 2012). The galaxy has a strong spiral structure that is excited by the satellite seen on the right of the image.
@rasjournals.bsky.socialOct 13, 2026, 8:48 AM

Published in #MNRAS: "Around the water snowline: I. Effects of dynamical and chemical interplay on mid-infrared water spectra of protoplanetary discs", Kaeufer et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Schematic representation of a protoplanetary disc (bottom) with a zoom-in (centre) onto the water snowline. Please visit the paper for the full caption.
@rasjournals.bsky.socialOct 12, 2026, 9:00 AM

Published in #MNRAS: "Life in the cosmic neighbourhood: galactic habitable zones in the EAGLE simulations", Barnes et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

The habitable time per unit baryonic mass (top) and per stellar mass (bottom), as a function of cosmic time (top axis) and redshift (bottom axis). Dashed lines show the predictions with no extinction events, while the solid line shows predictions will all extinctions. Please see the paper for the full caption.
@rasjournals.bsky.socialOct 9, 2026, 8:02 AM

Published in #MNRAS: "Galaxy populations in the IllustrisTNG caustic skeleton", Hertzsch et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

The dark and baryonic cosmic web in the TNG100 simulation of the IllustrisTNG suite. Please see the paper for the full caption.
@joseptrigo.bsky.socialOct 8, 2026, 7:57 PM

#Comet #220P McNaught imaged tonight after the cleaning rain experienced over #Catalonia the last week. Soon in #MNRAS our work on the 2 outbursts experienced since its perihelion, producing this fan of debris in a heterogenous clumpy tail & antitail🤩☄️
#MontsenyObservatory #S50 #PlanetaryScience

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@rasjournals.bsky.socialOct 8, 2026, 7:33 AM

Published in #MNRAS as a Letter: "The mysterious case of iron in XMPs: anomalous high log(Fe/O) observed in extremely metal-poor galaxies HSCJ1631+4426 and SDSSJ0811+4730", Myszka et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social

Composite RGB images of (a) HSCJ1631+4426 and (b) SDSSJ0811+4730. Please see the paper for the full caption.
@rasjournals.bsky.socialOct 7, 2026, 6:48 AM

Published in #MNRAS: "Highly bipolar planetary nebula Hen 2-57 and its possible symbiotic core", Merc et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

VPHAS + Halpha-r image of the nebula. North is up and East is left. The field shown is 72 arcsec x 72 arcsec.
@rasjournals.bsky.socialOct 6, 2026, 6:53 AM

Published in #MNRAS: "NGC 1901: a new benchmark cluster for gyrochronology in the TESS Southern continuous viewing zone", Bernizzoni et al. This is Fig. 2: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Observed colour–magnitude diagram of NGC 1901 showing core and tidal-tail members. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 25, 2026, 9:00 AM

Published in #MNRAS as a Letter: "Search for signatures of outflow interaction around Cygnus X-3", Martí et al. This is Fig. 6: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

NASA’s Wide-field Infrared Survey Explorer (WISE; E. L. Wright et al. 2010) trichromatic map (red 22 μm, green 12 μm, blue 3.4 µm) of CX3 field. The white dotted circle is the same as in Fig. 3, showing the suspected 7 arcmin H I cavity around CX3.
@rasjournals.bsky.socialSep 24, 2026, 8:45 AM

Published in #MNRAS: "The MICADO first light imager for the ELT: simulated observations of star forming clumps at cosmic noon", Simioni et al. This is Fig. 2: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Effect of different substructures of the host galaxy on clump detectability. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 23, 2026, 9:00 AM

Published in #MNRAS: "The MAGPI survey: emission-line products data release and the role of spectroscopic aperture covering fraction on the Balmer decrement–stellar mass relation", Battisti et al. Please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social

Sample MAGPI data. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 22, 2026, 8:13 AM

Published in #MNRAS: "Mergers lighting the early Universe: modest star formation enhancement without evidence for AGN or Lyα triggering", Puskás et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

An example galaxy pair system with its environment (top left) and three closely matched control systems. The primary galaxy is at the centre of each cutout, indicated by a red circle. The secondary galaxy in the pair system is indicated by a blue circle (only in the top-left cutout). Please see the paper for the full caption.
S@shashikiran.bsky.socialSep 22, 2026, 1:26 AM

Our paper on the post-perihelion photometric and spectroscopic studies of 3I/ATLAS is out on the arxiv now (accepted in MNRAS):

#3I/ATLAS #spectroscopy #MNRAS ☄️ #astrosci

arxiv.org/abs/2609.22596

@rasjournals.bsky.socialSep 21, 2026, 8:48 AM

Published in #MNRAS: "Analysis of the plane of satellites around Milky Way-mass galaxies in the IllustrisTNG simulation", Tang et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Local filament environment of Group 289 in the Cartesian y-slice passing through the halo centre, marked by the cross. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 18, 2026, 8:40 AM

Published in #MNRAS as a Letter: "Little Dots: the ULX analogy" by Andrew King. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Schematic picture of super-Eddington mass supply to a black hole, and the consequent differing radiation patterns for hard and soft X-ray emission. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 17, 2026, 8:48 AM

Published in #MNRAS: "The effect of the atmospheric C/O ratio on interiors of hot Jupiters", van Dijk et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Schematic illustration of the coupled interior-atmosphere model. Please see the paper for the full caption.
@rasjournals.bsky.socialSep 16, 2026, 7:15 AM

Published in #MNRAS: "The Stellar Populations of two quiescent low surface brightness dwarf galaxies in low-density environments", Forbes et al. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

DFUWS 68 (left) and DFUWS 258 (right). Please see the paper for the full caption.
@rasjournals.bsky.socialSep 15, 2026, 9:12 AM

Published in #MNRAS: "Formation of accretion disks around intermediate-mass black holes in ultra-compact dwarf galaxies and nuclear stellar clusters", Darr & Bekki. This is Fig. 1: please visit academic.oup.com/mnras/articl... to read the paper. @royalastrosoc.bsky.social @academic.oup.com

Schematic of the proposed mechanism for accretion disk formation and BH growth. The illustration presents the evolution of a UCD from a massive gas cloud to present-day UCDs with MBHs. The main idea presented is that the formation of AGB stars over time can undergo gas ejection which can infall towards an IMBH forming an accretion disk around it. The schematic also highlights key mechanisms present, such as the formation of new stars within the accretion disk that can populate the entire UCD. Leading to a key prediction for the proposed mechanism, being the creation of a new stellar population
@rasjournals.bsky.socialSep 14, 2026, 8:39 AM

Published in #MNRAS: "Planetary boundary-layer influence on optical turbulence at AlUla Manara", Alrefay et al. This is Fig. 2: please visit academic.oup.com/mnras/advanc... to read the paper.

The AlUla Manara Astronomical Site Monitor station. Visible in the frame are the 24hSHIMM optical turbulence monitor on its 8 m tower (left), the HATPRO microwave radiometer (centre, on a concrete pad), and the 30-m meteorological tower (right). The image is taken looking approximately east. Volcanic outcrops in the background are characteristic of the basalt plateau on which the site is located.