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RevMexAA (Serie de Conferencias), 14, 38--38 (2002) - The Mass Profile
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tracers. NGC 1399, the central galaxy of the Fornax cluster, is a particularly promising target for
www.astrosmo.unam.mx/rmaa/RMxAC..14/PDF/RMxAC..14_nstellar7.pdf
Unknown - The Astrophysical Journal
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"all-object" spectroscopic survey centered on the Fornax Cluster (Drinkwater et al. 2000, 2001)
155 astro.ph.unimelb.edu.au/mdrinkwa/fornax/papers/bekkiM32.pdf
astro.ph.unimelb.edu.au/mdrinkwa/fornax/ Unknown The Astrophysical Journal
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/bekkiM32.pdf
Cosmic Structure Traced by Precision - Measurements Of The
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A3266 EXO0422 N1550 A0478 A3158 IIIZw54 2A0335 FORNAX A3112 A0401 A0399 A0400 A0262 N507 A0133 A0119
astsun.astro.virginia.edu/~cls7i/papers/reiprich_maryland.ps.gz
Aa 376, 98--111 (2001) Doi: 10.1051/0004-6361:20010997 - Eso Astronomy Astrophysics
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&Astrophysics The neutral hydrogen content of Fornax cluster galaxies A. Schroder 1
of deep H i observations of member galaxies of the Fornax cluster. We detected 35 cluster galaxies in H i.
sample (0.05 0.03)Both these tests show that Fornax cluster galaxies are H i-deficient compared to
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/schroeder.pdf
Populations of Dwarfs in Clusters of Galaxies.. - Gallagher, Conselice..
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photographic studies of the Virgo and Fornax clusters by for example Bingelli et al. 1985)
Space Telescope, have recently resolved dEs in the Fornax and Virgo clusters, allowing us to chart their
in the near infrared, be extended to the Virgo and Fornax clusters. We wish to thank the National Science
www.astro.wisc.edu/prints/conselice/dge.ps.gz
THE ASTROPHYSICAL JOURNAL, 562 713726, 2001 December 1 V - The American Astronomical
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in Ferguson &Sandages (1989) sample of Virgo and Fornax galaxies show the same spatial distribution as
the Local Group. Galaxies like NGC 147, NGC 185, Fornax, Sextans, Leo I, Sagittarius, and Carina show
irregular galaxies and larger dEs like Phoenix, Fornax, WLM, Antlia, and NGC 205. This stresses the
astro.snu.ac.kr/~sckim/LGS3.web.pdf
The Luminosity Function of the Coma Cluster Core for - Gamma Gamma Bernstein
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work, Bothun et al. 1991) survey both Virgo and Fornax for LSB galaxies using photographic
!Gamma12. This is good news if true in Virgo and Fornax as well, because it means that there are not
appear at the distance of the Coma cluster (the Fornax galaxy is too bright to appear on this plot)
www.astro.lsa.umich.edu/users/garyb/PUBLICATIONS/ComaLF/comapp2.ps
Physical Sources of Scatter in the Tully-Fisher Relation - Kannappan, Fabricant, Franx
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drawn from a restricted environment. The Virgo and Fornax cluster samples of Yasuda et al. 1997) and
data from multiple clusters (including Ursa Major, Fornax, Coma, the Pisces Filament, and several others)
to a dierent degree. For example, the \complete" Fornax sample rejects interacting or disturbed galaxies
cfa-www.harvard.edu/~sheila/tfpaper.ps
The Fornax Spectroscopic Survey: The Number Of.. - Drinkwater.. (1999)
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All Rights Reserved. Printed In U.s.a. The Fornax Spectroscopic Survey: The Number Of Unresolved
( behind 18.5 !B !20.1 0.05 !z !0.21 J the Fornax Cluster. These galaxies are unresolved on UK
were found during initial observations of The Fornax Spectroscopic Survey. This project is using the
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/985628.web.pdf
The evolution and star formation of dwarf galaxies.. - Drinkwater, Gregg.. (2001)
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and star formation of dwarf galaxies in the Fornax Cluster M.J. Drinkwater 15 M.D. Gregg 23
J 18) galaxies in a 6 degree eld centred on the Fornax cluster with the FLAIR-II spectrograph on the UK
for 516 galaxies of which 108 were members of the Fornax Cluster. De ning dwarf galaxies to be those with
astro.ph.unimelb.edu.au/~mdrinkwa/papers/fornax_flair2.ps.gz
On the Formation of Galaxy Halos: Comparing NGC 5128 and .. - William Harris..
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Guhathakurta 1999)the SMC (Larsen et al. 2000)Fornax (Saviane et al. 2000)Sagittarius (Bellazzini et
physun.mcmaster.ca/~harris/Publications/ngc5128.ps
Substructure And Dynamics Of The Fornax Cluster - Michael Drinkwater School
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Printed In U.s.a. Substructure And Dynamics Of The Fornax Cluster Michael J. Drinkwater School Of
fraction of dwarf galaxies. Our sample of 108 Fornax Cluster members measured with the UK Schmidt
objects whereas the giants are virialized. The Fornax system has two components, the main Fornax
astro.ph.unimelb.edu.au/~mdrinkwa/papers/fornax_flair3.pdf
The Mass of the Milky Way - Oiwei Ivy Wong
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velocity using high-velocity stars taken from the Fornax Spectroscopic Survey (hereafter FSS)This is the
area of 2 degree 2 in the region of the Fornax cluster (Drinkwater et al. 2000)Of these 7000
. 5 2 High-Velocity Star Sample 6 2.1 2dF Fornax Spectroscopic Survey .
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/wong_thesis.ps.gz
Extragalactic Seti And The Uws/atnf/serendip Project - Ray Norris Csiro
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Dec(B1950) Target #Sculptor 00 57.5-33 58 9051 Fornax 02 37.1-34 44 9052 Leo I 10 05.8 12 33 9053 NGC
www.atnf.csiro.au/~rnorris/papers/n157.ps
Ultracompact Dwarf Galaxies In The Fornax Cluster - Phillipps, al. (2001)
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In U.s.a. Ultracompact Dwarf Galaxies In The Fornax Cluster S. Phillipps Astrophysics Group,
area toward the center of 16.5 \b j 19.7, the Fornax Cluster of galaxies. Among the unresolved or
objects that are actually at the redshift of the Fornax Cluster i.e.they are extremely compact dwarf
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/apj_ucd.pdf
High surface brightness dwarf galaxies in the Fornax cluster - Michael Drinkwater And
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High surface brightness dwarf galaxies in the Fornax cluster Michael J. Drinkwater 1 and Michael
a search for compact dwarf galaxies in the Fornax cluster using the FLAIR spectrograph on the UK
have been conducting a spectroscopic survey of the Fornax cluster using the UK Schmidt Telescope (UKST)
astro.ph.unimelb.edu.au/~mdrinkwa/papers/seven_mnras.ps.gz
Low Surface Brightness Galaxies in the Core of the.. - Ulmer, Bernstein.. (1996)
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those found by others in nearby clusters such as Fornax (Bothun, Impey &Malin)as well as in the low
denser cluster environments than previous reports: Fornax (Bothun, Impey &Malin 1991 Bothun, Caldwell &
see Bothun et al. 1989)3.2. Comparison with Fornax and Virgo To provide more details, as well as to
www.astro.lsa.umich.edu/users/garyb/PUBLICATIONS/ComaLSB/mel.ps
The Fornax spectroscopic survey - Survey Strategy And
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900-914 (2000) Astronomy And Astrophysics The Fornax Spectroscopic Survey I. Survey Strategy And
1999 /Accepted 25 January 2000 Abstract. The Fornax Spectroscopic Survey will use the Two degree
19.7 in a 12 square degree area centred on the Fornax Cluster. The aims of this project include the
astro.ph.unimelb.edu.au/~mdrinkwa/fornax/papers/2300900.pdf
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