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1. Classification of Wolf–Rayet Stars Using Ensemble-based Machine Learning Algorithms.

2. The Rise of Nova V1674 Herculis.

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3. A Modified Initial Mass Function of the First Stars with Explodability Theory under Different Enrichment Scenarios.

4. Super-slowly rotating Ap (ssrAp) stars: Spectroscopic study.

5. The symbiotic recurrent nova V745 Sco at radio wavelengths.

6. FitteR for Accretion ProPErties of T Tauri stars (FRAPPE): A new approach to use class III spectra to derive stellar and accretion properties.

7. V407 Lup, an intermediate polar nova.

8. A phenomenological study of the evolution of shock-induced O i emission lines in the spectrum of nova V2891 Cygni.

9. More Luminous Red Novae That Require Jets.

10. I-band photometry of the quiescent black hole X-ray nova GROJ0422 + 32 = V518 Per: modelling of the orbital light curve and estimation of the black hole mass.

11. Modifying the Health Star Rating nutrient profiling algorithm to account for ultra‐processing.

12. DAVID KONSTAN, LA AMISTAD COMO ENSEÑANZA: IN MEMORIAM.

13. A dusty rain falls on the nova V959 Monocerotis.

14. The SARAO MeerKAT 1.3 GHz Galactic Plane Survey.

15. 3D physical structure and angular expansion of the remnant of the recurrent nova T Pyx.

16. Evidence of the γ-ray counterpart of nova FM Cir from Fermi–LAT.

17. Gaia23ckh: Symbiotic outburst of the assumed Mira variable V390 Sco.

18. The Hybrid Nova V1405 Cas with an Oxygen–Neon or Carbon–Oxygen White Dwarf?

19. Studying lepton flavor violating μ decays with vector leptoquark.

20. Under the light of a new star: evolution of planetary atmospheres through protoplanetary disc dispersal and boil-off.

21. Neutron star mergers as the dominant contributor to the production of heavy r-process elements.

22. Optical and soft X-ray light-curve analysis during the 2022 eruption of U Scorpii: Structural changes in the accretion disk.

23. The peculiar bursting nature of CP Pup.

24. Introducing the Condor Array Telescope – IV. A possible nova super-remnant surrounding the putative recurrent nova KT Eridani.

25. Introducing the Condor Array Telescope – III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell.

26. Hydrodynamic simulations of the KT Eridani nova super-remnant.

27. Shock-driven synchrotron radio emission from the 2021 outburst of RS Ophiuchi.

28. Discovery of a nova super-remnant cavity surrounding RS Ophiuchi.

29. On an apparent dearth of recurrent nova super-remnants in the Local Group.

30. Soft X-ray and FUV observations of Nova Her 2021 (V1674 Her) with AstroSat.

31. Exploration of faint X-ray and radio sources in the massive globular cluster M14: a UV-bright counterpart to Nova Ophiuchus 1938.

32. LAMOST J040901.83+329355.6 – a new Galactic star with Wolf–Rayet characteristics in the transitional stage from post-asymptotic giant branch to central star of a planetary nebula.

33. TESS Cycle 2 observations of roAp stars with 2-min cadence data.

34. Study of the Rapid Variability of a Dwarf Nova SS Cyg at Different Brightness Levels.

35. Get Ready for a Nova's Bright Return: Recurrent nova T Coronae Borealis last erupted in 1946. It's due to erupt again this year.

36. A new star formation recipe for magnetohydrodynamics simulations of galaxy formation.

37. A two-component clumpy model for the shell evolution of classical novae: the case of V5668 Sgr.

38. Eruptive novae in symbiotic systems.

39. Revisiting the classics: on the evolutionary origin of the 'Fe ii' and 'He/N' spectral classes of novae.

40. Magnetic field effects on nucleosynthesis and kilonovae from neutron star merger remnants.

41. Contributing to the spectral evolution of the nova V1405 Cas.

42. Study of the fastest classical nova, V1674 Her: photoionization and morpho-kinemetic model analysis.

43. A search for extragalactic fast optical transients in the Tomo-e Gozen high-cadence survey.

44. On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos.

45. The orbital period of the recurrent nova V2487 Oph revealed.

46. A multimessenger model for neutron star–black hole mergers.

47. The NOVA Mobile Planetarium: Ten best practices for planetarium projects based on an astronomy education success story.

48. The recurrent nova T CrB had prior eruptions observed near December 1787 and October 1217 AD.

49. TESS light curves of cataclysmic variables – III – More superhump systems among old novae and nova-like variables.

50. Orbital period changes for 14 novae and the critical failures of the predictions of standard theories, the Hibernation Model, and the Magnetic Braking Model.