We present minor axis kinematic profiles for a well-studied sample of 19 early- to intermediate-type disk galaxies. We introduce, for the first time, the use of...
Mirach's Goblin: Discovery of a dwarf spheroidal galaxy behind the Andromeda galaxy
Context. It is of broad interest for galaxy formation theory to carry out a full inventory of the numbers and properties of dwarf galaxies, both satellite and...
MIRACLE: I. Unveiling the multi-phase, multi-scale physical properties of the active galaxy NGC 424 with MIRI, MUSE, and ALMA
We present an analysis of the multi-phase gas properties in the Seyfert II galaxy NGC 424, using spatially resolved spectroscopic data from JWST/MIRI, part of...
MIRACLE: II. Unveiling the multiphase gas interplay in the circumnuclear region of NGC 1365 via multicloud modeling
We present a multiphase analysis of the gas in the circumnuclear region (∼0.9 × 0.9 kpc 2) of the nearby barred Seyfert 1.8 galaxy NGC 1365, observed as part of...
Misaligned spin-orbit in the XO-3 planetary system?
The transiting extrasolar planet XO-3b is remarkable, with a high mass and eccentric orbit. These unusual characteristics make it interesting to test whether...
Missing dust of super-early galaxies: Supernova blowout and gas─dust venting in blue monsters
Context. A subset of very young super-early galaxies at z ≳ 10, often called blue monsters, shows extremely blue UV continua and faint far-IR emission. This...
Missing large-angle correlations versus even-odd point-parity imbalance in the cosmic microwave background
Context. The existence of a maximum correlation angle (θ max ≳ 60°) in the two-point angular temperature correlations of cosmic microwave background (CMB)...
Mixing by internal waves. III. Li and Be abundance dependence on spectral type, age and rotation
In this paper we deal with the problem of the generation of internal waves at the bottom of convective zone in solar-type stars, and with the transport process...
MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals
Aims. We examined the anomalies in the light curves of the lensing events MOA-2022-BLG-033, KMT-2023-BLG-0119, and KMT- 2023-BLG-1896. These anomalies share...