Search Publications

Galaxy Threshing and Ultra-Compact Dwarfs in the Fornax Cluster
DOI: 10.1023/A:1024622128955 Bibcode: 2003Ap&SS.285..113G

Ferguson, Henry C.; Phillipps, Steven; Drinkwater, M. J. +3 more

We have discovered a new type of galaxy in the Fornax Cluster: `ultra-compact' dwarfs (UCDs). The UCDs are unresolved in ground-based imaging and have spectra typical of old stellar systems. Although the UCDs resemble overgrown globular clusters, based on VLT UVES echelle spectroscopy, they appear to be dynamically distinct systems with higher int…

2003 Astrophysics and Space Science
eHST 8
Photometric studies of very metal-deficient blue compact dwarf galaxies: the exponential ionized gas halo of IZw18
DOI: 10.1023/A:1024022409637 Bibcode: 2003Ap&SS.284..619P

Thuan, T. X.; Izotov, Y. I.; Papaderos, P. +4 more

Using HST and ground-based optical and NIR imaging data, we investigate whether the blue compact dwarf (BCD) galaxy I Zw 18 possesses an extended low-surface brightness (LSB) old stellar population underlying its star-forming (SF) regions. We show that the exponential intensity decrease observed in the filamentary LSB envelope of the BCD out to 18…

2003 Astrophysics and Space Science
eHST 3
Tidal dwarfs in the M81 group: the second generation?
DOI: 10.1023/A:1024670028046 Bibcode: 2003Ap&SS.285..107M

Sarajedini, A.; Geisler, D.; Guhathakurta, P. +8 more

We present a quantitative star formation history derivation of the four suspected tidal dwarf galaxies in the M 81 group: Holmberg IX, BK3N,Arp-loop (A0952+69) and Garland using HST/WFPC2 images of these galaxies. We construct a library of synthetic Colour-Magnitude Diagrams(CMDs) based on theoretical isochrones and data-derived determinations of …

2003 Astrophysics and Space Science
eHST 3
The extended structure of the Phoenix dwarf galaxy
DOI: 10.1023/A:1024010106912 Bibcode: 2003Ap&SS.284..595H

Aparicio, Antonio; Hidalgo, Sebastian L.; MartÍnez-Delgado, David

The surface brightness profile in the V band of the Phoenix dwarf galaxy shows two stellar components: an inner one, which contains all the young stars of the galaxy, and an outer one predominantly populated by red stars. Deep color-magnitude diagrams (CMDs), based on Hubble Space Telescope (HST) observations and reaching the oldest turn-offs, are…

2003 Astrophysics and Space Science
eHST 3
The resolved red giant branches of E/S0 galaxies
DOI: 10.1023/A:1024083220618 Bibcode: 2003Ap&SS.284..909S

Hopp, Ulrich; Schulte-Ladbeck, Regina E.; Drozdovsky, Igor O. +1 more

Formation paradigms for massive galaxies have long centered around two antipodal hypotheses – the monolithic-collapse and the accretion/merger scenarios. Empirical data on the stellar contents of galaxy halos is crucial in order to develop galaxy formation and assembly scenarios which have their root in observations, rather than in numerical simul…

2003 Astrophysics and Space Science
eHST 3
Tests and constraints on theories of galaxy formation and evolution
DOI: 10.1023/A:1024034228409 Bibcode: 2003Ap&SS.284..353T

Thompson, Rodger I.

Tests and constraints on current theories of galaxy formation and evolution are presented. They are derived from observations of the Northern Hubble Deep Field with WFPC2 and NICMOS. Photometric redshifts, extinctions and spectral energy distributions are calculated for all objects in the field. The tests and constraints are derived from the outpu…

2003 Astrophysics and Space Science
eHST 3
A survey searching for the epoch of assembling of Hubble types
DOI: 10.1023/A:1024006900184 Bibcode: 2003Ap&SS.284..389D

Pasquali, Anna; de Mello, DuÍlia F.

We have started a survey of galaxies at intermediate redshifts using the HST-STIS parallel fields. Our main goal is to analyse the morphology of faint galaxies in order to estimate the epoch of formation of the Hubble classification sequence. The high resolution of STIS images (0.05″) is ideal for this work and enables us to perform a morphologica…

2003 Astrophysics and Space Science
eHST 0