Journal: Monthly Notices of the Royal Astronomical Society
Publication
Complex emission line region of Mrk 817
In this work, we study the physical and kinematical properties of the emission line region of the Seyfert 1.5 galaxy Mrk 817 using three sets of observations...
Complex particle acceleration processes in the hotspots of 3C 105 and 3C 445
We investigate the nature of the broad-band emission associated with the low-power radio hotspots 3C 105 South and 3C 445 South. Both hotspot regions are...
Component masses of young, wide, non-magnetic white dwarf binaries in the Sloan Digital Sky Survey Data Release 7
We present a spectroscopic component analysis of 18 candidate young, wide, non-magnetic, double-degenerate binaries identified from a search of the Sloan...
Composite bulges - II. Classical bulges and nuclear discs in barred galaxies: the contrasting cases of NGC 4608 and NGC 4643
We present detailed morphological, photometric, and stellar-kinematic analyses of the central regions of two massive, early-type barred galaxies with nearly...
Composite bulges: the coexistence of classical bulges and discy pseudo-bulges in S0 and spiral galaxies
We present an analysis of nine S0-Sb galaxies which have (photometric) bulges consisting of two distinct components. The outer component is a flattened...
Compositional characterization of V-type candidate asteroids identified using the MOVIS catalogue
The main objective of this work is to compositionally analyse the visible to near-infrared spectra of a total of six V-type candidates identified using the...
Comprehensive analytic formulae for stellar evolution as a function of mass and metallicity
We present analytic formulae that approximate the evolution of stars for a wide range of mass M and metallicity Z. Stellar luminosity, radius and core mass are...
Concerning colour: The effect of environment on type Ia supernova colour in the dark energy survey
Recent analyses have found intriguing correlations between the colour (c) of type Ia supernovae (SNe Ia) and the size of their 'mass-step', the relationship...
Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae
It has recently been noted that there seems to be a strong correlation between planetary nebulae with close binary central stars and highly enhanced...