The k luminosity-metallicity relation for dwarf galaxies and the tidal dwarf galaxies in the tails of hcg 31.

• Grant number: 07/00179-0
• Support Opportunities: Regular Research Grants - Publications - Scientific article
• Start date: February 01, 2007
• End date: April 30, 2007
• Field of knowledge: Physical Sciences and Mathematics - Astronomy - Extragalactic Astrophysics
• Principal Investigator: Laerte Sodré Junior
• Grantee: Laerte Sodré Junior
• Host Institution: Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG). Universidade de São Paulo (USP). São Paulo , SP, Brazil

Abstract

We determine the first fossil group luminosity function based on spectroscopy of the member galaxies. The fossil group RX J1552.2+2013 has 36 confirmed members, is at a mean redshift of 0.136, and has a velocity dispersion of 623 km/s. The luminosity function of RX J1552.2+2013, measured within the inner region of the system, is well fitted by a Schechter function with M*i'=-21.3 and alpha=-0.6 or by a Gaussian function centered on Mi'=-20.0 with sigma=1.29 i' mag. The luminosity function obtained from a photometric survey in the g', r', and i' bands (and statistical background correction) confirms the spectroscopically determined results. There is a significant dip in the luminosity function at Mr'=-18 mag, as is also observed for other clusters. RX J1552.2+2013 is a rich, red-galaxy-dominated system, with at least 19 galaxies with magnitudes between m3 and m3+2, within a surveyed circular area of radius 625 kpc centered on the peak of the X-ray emission. Its mass, ~3×10^14 Msolar, M/L of 507 Msolar/LBsolar, and LX of 6.3×10^43 erg/s (bolometric) are more representative of a fossil cluster than of a fossil group. The central object of RX J1552.2+2013 is a cD galaxy that may have accreted the more luminous (~L*) former members of the group. Although dynamical friction and subsequent merging are probably the processes responsible for the lack of bright galaxies in the system, for the fainter members there must be another mechanism in action (perhaps tidal disruption) to deplete intermediate-luminosity galaxies (Mr'~-18) from the fossil group. (AU)