ar X iv : a st ro - p h / 01 07 42 5 v 1 2 1 Ju l 2 00 1 Star Formation in the Interacting Pair NGC 7733 / 34

ar X iv : a st ro - p h / 01 07 35 5 v 1 1 8 Ju l 2 00 1 Global star formation history : A Local Group perspective

The global star formation rate (SFR) density is estimated from the star formation histories (SFHs) of Local Group galaxies. This is found to be broadly consistent with estimates of the global SFH from existing redshift surveys for two favoured cosmologies. It also provides additional evidence for a relatively constant global SFR density at high redshift (z > 1).

ar X iv : a st ro - p h / 02 10 42 8 v 1 1 8 O ct 2 00 2 Star Clusters in Interacting Galaxies : The Case of M 51 Nate

ar X iv : a st ro - p h / 02 10 42 0 v 1 1 8 O ct 2 00 2 Extragalactic Globular Clusters in the Near - Infrared

Visual and near-infrared colours are used to identify intermediate-age globular cluster in early-type galaxies. In NGC 5846 and NGC 4365 colour-colour diagrams (V-I vs. V-K) reveal a sub-population in the globular cluster systems with an age much younger than the expected old populations (13-15 Gyr). A comparison with SSP models dates the formation of this younger population 2-7 Gyr back. Furth...

ar X iv : a st ro - p h / 99 06 25 1 v 1 1 5 Ju n 19 99 Inflow and outflows in NGC 2992 / 3

We present observational evidences for inflow and outflows in the interacting system Arp 245 (NGC 2992/3).

ar X iv : a st ro - p h / 05 08 67 7 v 1 3 1 A ug 2 00 5 CONTINUOUS STAR CLUSTER FORMATION IN THE SPIRAL NGC 45

We determined ages for 52 star clusters with masses ≤ 10 M⊙ in the low surface brightness spiral galaxy NGC 45. Four of these candidates are old globular clusters located in the bulge. The remaining ones span a large age range. The cluster ages suggest a continuous star/cluster formation history without evidence for bursts, consistent with the galaxy being located in a relatively unperturbed en...