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A Supergroup in 6dFGS

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A key prediction of hierarchical structure formation is that galaxy clusters ... Examine substructure in Eridanus group. Study morphological mix of region. ... – PowerPoint PPT presentation

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Title: A Supergroup in 6dFGS


1
A Supergroup in 6dFGS
Piccy here
  • Sarah Brough, Swinburne University
  • Virginia Kilborn, Duncan Forbes, Swinburne
    University
  • Warrick Couch, UNSW
  • Heath Jones, Mount Stromlo
  • Matthew Colless, AAO

2
  • A key prediction of hierarchical structure
    formation is that galaxy clusters assemble at
    late times from the merging and accretion of
    smaller structures (e.g. Peebles 1970).
  • We lack clear early-stage examples of clusters
    being assembled from an ensemble of galaxy
    groups.
  • Two of the groups in the GEMS sample (NGC 1332
    and NGC 1407) are associated with a much larger
    system the Eridanus cloud

3
Eridanus - a Supergroup?
  • Eridanus is a cloud of galaxies 23 Mpc away
    (Baker 1933,1936 de Vaucouleurs 1975)
  • Forms a filamentary structure with the Fornax
    cluster (da Costa et al. 1988).
  • There is intra-group X-ray emission around NGC
    1395 and NGC 1407, but not NGC 1332.

NGC 1407
NGC 1332
Eridanus
Fornax
4
X-Ray Images
Osmond Ponman (2004)
Omar Dwarakanath (2005)
Osmond Ponman (2004)
5
Advent of 6dFGS
  • The 6dFGS database provides a unique source of
    positions, velocities, 2MASS near-IR magnitudes
    and spectra with which to analyse the properties
    of this region in detail.
  • Galaxies with velocities lt 2500 km s-1
  • 470 NED sources
  • 114 new 6dFGS sources
  • 249 total sources in Eridanus region (25 more
    than NED).

NGC 1407
NGC 1332
Eridanus
Fornax
6
Previous Work
  • Willmer et al (1989) studied 139 galaxies in the
    region, concluding that Eridanus is a cluster
    with 3-4 sub-clumps (around NGC 1332, NGC 1395
    and NGC 1407) each with different morphological
    mixes. They determined that these are all bound
    and will merge to form a 1013 M? cluster.
  • Omar Dwarakanath (astro-ph/0503536) studied 181
    galaxies in the region and claim that the
    properties of Eridanus indicate that it is at an
    evolutionary stage intermediate to that of the
    field and a cluster of galaxies.

7
FOF Determined Groups
  • In order to study region need to define which
    galaxies are associated with which
    sub-clump/group/cluster.
  • Use friends-of-friends technique (Huchra Geller
    1982)
  • Following the prescriptions of 2dF (Eke et al.
    2004)
  • ????? 150
  • 2??r 1200

NGC 1407
NGC 1332
Eridanus
8
Velocity Distribution
9
Derived Properties
10
Brightest Group Galaxies
  • Galaxy at centre of structure gives some clue as
    to evolutionary status.
  • No bright, centrally-dominant galaxy or X-ray
    emission at centre of Eridanus group
  • Large elliptical at centre of NGC 1407 group and
    X-ray emission.
  • Luminosity weighted centre and mean velocity of
    group correspond to those of NGC 1407.

11
Neutral Hydrogen Content
  • Omar Dwarakanath (2005) conclude that galaxies
    in the highest density regions are deficient in
    HI by a factor of 2-3 as a result of tidal
    interactions
  • We observe that are no HI sources within NGC 1407
    but several within NGC 1332 groups.

NGC 1407
NGC 1332
Kilborn et al. in prep
12
Colour Distributions
  • Kodama et al. 2002 observe bimodality in colours
    of galaxy populations dependent on their
    environment.
  • This region spans a dense cluster, groups,
    filaments and the field.
  • Obtained B mags from Hyper-leda, resulting in
    225/536 galaxies with B-K colours.

Median
Fornax
NGC 1407
NGC 1332
NGC 1395
13
High Density (43 galaxies) Low Density (182
galaxies)
14
NGC 1407
NGC 1332
NGC 1395
15
Future Directions
  • Analyse whether groups are infalling and on what
    timescale.
  • Compare observations with N-body simulations.
  • Examine substructure in Eridanus group.
  • Study morphological mix of region.
  • Obtain star formation rates from 6dF spectra.

16
Summary
  • NGC 1407 is a massive group at a late stage in
    group evolution.
  • Eridanus appears to be made up of 2 sub-groups
    each at an early stage of their evolution.
  • These groups will coalesce to form a cluster of
    mass 6x1013 M?. The individual BGGs will merge
    to form a large central elliptical (Brough et al.
    2002 Lin Mohr 2004).
  • The colours of the individual galaxies indicate
    that this structure straddles the density around
    which any galaxy transformation is occurring.
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