Journal: Monthly Notices of the Royal Astronomical Society
Publication
Ages of LMC star clusters using ASAD2
We use ASAD2, the new version of ASAD (Analyzer of Spectra for Age Determination), to obtain the age and reddening of 27 Large Magellanic Cloud (LMC) clusters...
AGN feedback and star formation in the peculiar galaxy NGC 232: insights from VLT-MUSE observations
We use VLT-MUSE integral field unit data to study the ionized gas physical properties and kinematics as well as the stellar populations of the Seyfert 2 galaxy...
We present the most complete atlas of nuclear rings to date. We include 113 rings found in 107 galaxies, six of which are elliptical galaxies, five are highly...
AlH lines in the blue spectrum of Proxima Centauri
The recently computed ExoMol line lists for isotopologues of AlH are used to analyse the blue spectrum (4000-4500 Å) of Proxima Cen (M5.5 V). Comparison of the...
ALMA High-Level Data Products: submillimetre counterparts of SDSS quasars in the ALMA footprint
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world's most advanced radio interferometric facility, producing science data with an average rate...
ALMA reveals a compact and massive molecular outflow driven by the young AGN in a nearby ULIRG
The ultraluminous infrared galaxy F13451+1232 is an excellent example of a galaxy merger in the early stages of active galactic nucleus (AGN) activity, a phase...
Alone on a wide wide sea. The origin of SECCO 1, an isolated star-forming gas cloud in the Virgo cluster*†‡
SECCO 1 is an extremely dark, low-mass (M⋆ ≃ 105 M⊙), star-forming stellar system lying in the low-velocity cloud (LVC) substructure of the Virgo cluster of...
Amino acids in comets and meteorites: stability under gamma radiation and preservation of the enantiomeric excess
Amino acids in Solar system bodies may have played a key role in the chemistry that led to the origin of life on Earth. We present laboratory studies testing...
An active M8.5 dwarf wide companion to the M4/DA binary LHS 4039/LHS 4040
Low-mass and brown dwarfs have recently been found as wide companions to many nearby stars, formerly believed to be single. Wide binaries are usually found as...