In order to definitely prove the claim by Claeskens et al. (1996A&A...305L...9C) that J03.13 is a doubly imaged quasar, WFPC2 direct imaging and FOS...
HST grism spectroscopy of z ∼ 3 massive quiescent galaxies. Approaching the metamorphosis
Tracing the emergence of the massive quiescent galaxy (QG) population requires the build-up of reliable quenched samples by distinguishing these systems from...
HST/ACS observations of shell galaxies: inner shells, shell colours and dust
Context: Shells in Elliptical Galaxies are faint, sharp-edged features, believed to provide evidence for a merger event. Accurate photometry at high spatial...
Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves
The merger of two compact objects of which at least one is a neutron star is signalled by transient electromagnetic emission in a kilonova (KN). This event is...
Hubble Space Telescope study of resolved red giant stars in the outer halos of nearby dwarf starburst galaxies
Context. Central starbursts in galaxies are an extreme example of ongoing galaxy evolution. The outer parts of galaxies contain a fossil record of galaxy...
Hubble spectroscopy of LB-1: Comparison with B+black-hole and Be+stripped-star models
Context. LB-1 (alias ALS 8775) has been proposed as either an X-ray dim B-type star plus black hole (B+BH) binary or a Be star plus an inflated stripped star...
Hunting for anti-solar differentially rotating stars using the Rossby number. An application to the Kepler field
Context. Anti-solar differential rotation profiles have been found for decades in numerical simulations of convective envelopes of solar-type stars. These...
Hydride ion continuum hides absorption signatures in the NIRPS near-infrared transmission spectrum of the ultra-hot gas giant WASP-189b
Context. Ultra-hot Jupiters showcase one-of-a-kind extreme atmospheric conditions, including the dissociation of molecules into atomic species, ionisation, and...
Hydrodynamic simulations of cool stellar atmospheres with MANCHA
Context. Three-dimensional time-dependent simulations of stellar atmospheres are essential to study the surface of stars other than the Sun. These simulations...