Bibcode
Phillips, A. C.; Guzman, R.; Gallego, J.; Lowenthal, J. D.; Vogt, N. P.; Koo, D.; Faber, S.; Illingworth, G.
Referencia bibliográfica
American Astronomical Society, 189th AAS Meeting, #103.08; Bulletin of the American Astronomical Society, Vol. 28, p.1413
Fecha de publicación:
12
1996
Número de citas
1
Número de citas referidas
1
Descripción
We present Keck spectroscopy of small (r<0.5('') ), high surface
brightness galaxies in the flanking fields of the Hubble Deep Field. The
spectroscopic data is used along with HST images to provide redshift
distributions, luminosities, physical sizes, mass estimates and
star-formation rates. We find the sample consists mostly of emission
line galaxies, with a significant fraction ( ~ 25%) of early-type
systems. Only a few galaxies in the sample are obvious AGNs or z>2
objects. The majority of the emission-line systems have properties
similar to local Hii galaxies.