Are disappearing dwarfs just lying low ?
arXiv:astro-ph/9511133 · doi:10.1093/mnras/274.3.832
Abstract
Recent redshift surveys have shown that the excess galaxies seen in faint galaxy number counts (above those expected given the local galaxy luminosity function) are not evolved giants at high redshifts, but low to moderate luminosity objects at more modest redshifts. This has led to the suggestion that there was once an additional population of dwarf galaxies which has since disappeared, ie. there is non-conservation of galaxy number. Here we investigate the possibility that these disappearing dwarfs have actually evolved to become the population of very low surface brightness galaxies which is now being detected in nearby clusters.
12 pages, 7 figures. Figures available from http://www.phys.unsw.edu.au/~spd/bib.html
Cited by in corpus (30)
- The Impact of Star Formation on the Interstellar Medium in Dwarf Galaxies: II. The Formation of Galactic Winds
- Faint Blue Galaxies
- The Nature of Compact Galaxies in the Hubble Deep Field (II): Spectroscopic Properties and Implications for the Evolution of the Star Formation Rate Density of the Universe
- The Millennium Galaxy Catalogue: 16 < B_MGC < 24 galaxy counts and the calibration of the local galaxy luminosity function
- Galaxy number counts - V. Ultra-deep counts: The Herschel and Hubble Deep Fields
- Gas Mass Fractions and the Evolution of Spiral Galaxies
- The morphological mix of field galaxies to I=24.25 magnitudes (b=26 magnitudes) from a deep Hubble Space Telescope WFPC2 image
- The Millennium Galaxy Catalogue: the space density and surface brightness distribution(s) of galaxies
- Morphological number-count and redshift distributions to I < 26 from the Hubble Deep Field: Implications for the evolution of Ellipticals, Spirals and Irregulars
- Spectral Classification and Luminosity Function of Galaxies in the Las Campanas Redshift Survey
- The 2dF Galaxy Redshift Survey: The Number and Luminosity Density of Galaxies
- New limits on a cosmological constant from statistics of gravitational lensing
- Galaxy And Mass Assembly (GAMA): ugrizYJHK Sérsic luminosity functions and the cosmic spectral energy distribution by Hubble type
- Young Clusters in the Nuclear Starburst of M 83
- Shedding Light on the Galaxy Luminosity Function
- The Photometric Redshift Distribution and Evolutionary Properties of Galaxies up to z= 4.5 in the Field of the Quasar BR1202-0725
- A Near-Infrared Stellar Census of Blue Compact Dwarf Galaxies: The Wolf-Rayet Galaxy I Zw 36
- The Ccontribution of normal, dim and dwarf galaxies to the local luminosity density
- The Luminosity Distribution in Galaxy Clusters: A Dwarf Population - Density Relation?
- Deep Luminosity Functions and Colour-Magnitude Relations for Cluster Galaxies at 0.2 < z < 0.6
- The ugrizYJHK luminosity distributions and densities from the combined MGC, SDSS and UKIDSS LAS datasets
- Systematic Biases in Galaxy Luminosity Functions
- Cloning Hubble Deep Fields II: Models for Evolution by Bright Galaxy Image Transformation
- A Look At Three Different Scenarios for Bulge Formation
- GOYA Survey: U and B Number Counts in the Groth-Westphal Strip
- The Sheet of Giants: Unusual Properties of the Milky Way's Immediate Neighbourhood
- Morphological evolution in situ: Disk-dominated cluster red sequences at z ~ 1.25
- An Emission-Line Search for Star-Forming Dwarf Galaxies Toward Abell 851
- The History of Galaxies and Galaxy Number Counts
- The inferred redshift distribution of the faint blue excess