Can galaxy outflows and re-accretion produce the downsizing in specific star formation rate of late-type galaxies?
arXiv:0909.5188 · doi:10.1111/j.1365-2966.2010.16366.x
Abstract
The observations show that less massive the galaxies are, the higher on average is their specific star formation rate (SSFR = SFR/Ms, Ms is the stellar mass). Such a trend, called the 'SSFR downsizing' (SSFR-DS) phenomenon, is seen for local and high-z (back to z~1-2) galaxy samples. We use observational data related only to disc galaxies and explore the average SSFR change with z for different masses. For Ms in the range ~10^9.5-10^10.5 Msun, the SSFR increases with (1+z) to a power that barely depends on Ms, and at all z's smaller galaxies have ever higher SSFRs. The latter strongly disagree with the LCDM hierarchical mass accretion rates. By means of self-consistent models of disc galaxy evolution inside growing LCDM halos, the effects that disc feedback-driven outflows and gas re-accretion have on the galaxy SSFR histories are explored. The parameters of the outflow and re-accretion schemes are tuned to reproduce the z~0 Mh-Ms relation inferred from observations. In the case of outflows only, the SSFR of individual model galaxies is roughly proportional to (1+z)^2.2 for all the masses with a normalization factor that depends on mass as Ms^0.1, i.e more massive galaxies have slightly larger SSFRs, contrary to the observed strong SSFR-DS trend. For the re-accretion cases, the dependence on z remains approximately the same as without re-infall, but the correlation on Ms even increases for most of the reasonable values of the model parameters. The comparison of models and observations in the SSFR-Ms plane at z~0 shows the divergent trend in SSFR as lower are the masses (upsizing vs downsizing). We explain why the models show the reported trends, and conclude that the SSFR-DS for low-mass galaxies poses a challenge for LCDM-based disc galaxy evolution models. (Abridged)
12 pages, 4 figures. To appear in MNRAS. Text improved after Referee reports
References in corpus (30)
- Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- UV Star Formation Rates in the Local Universe
- Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
- The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
- Mass, Metal, and Energy Feedback in Cosmological Simulations
- The Origin of the Galaxy Mass-Metallicity Relation and Implications for Galactic Outflows
- Star formation in AEGIS field galaxies since z=1.1 . Staged galaxy formation, and a model of mass-dependent gas exhaustion
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
- Evidence for TP-AGB stars in high redshift galaxies, and their effect on deriving stellar population parameters
- The UV-Optical Color Magnitude Diagram II: Physical Properties and Morphological Evolution On and Off of a Star-Forming Sequence
- The star formation histories of galaxies in the Sloan Digital Sky Survey
- On the onset of galactic winds in quiescent star forming galaxies
- Natural Downsizing in Hierarchical Galaxy Formation
- The MORGANA model for the rise of galaxies and active nuclei
- The propagation of uncertainties in stellar population synthesis modeling II: The challenge of comparing galaxy evolution models to observations
- Galaxy growth in the concordance CDM cosmology
- Star Formation and the Growth of Stellar Mass
- The dependence of Star Formation on Galaxy Stellar Mass
- The Impact of Feedback on Disk Galaxy Scaling Relations
- The recycling of gas and metals in galaxy formation: predictions of a dynamical feedback model
- The evolution of the specific star formation rate of massive galaxies to z ~ 1.8 in the E-CDFS
- The Properties and Evolution of a K-band Selected Sample of Massive Galaxies at z~0.4 - 2 in the Palomar/DEEP2 Survey
- The Star Formation Demographics of Galaxies in the Local Volume
- On the baryonic, stellar, and luminous scaling relations of disk galaxies
- The Star Formation and Extinction Co-Evolution of UV-Selected Galaxies over 0.05<z<1.2
- Faint Lyman-Break galaxies as a crucial test for galaxy formation models
- Constraints on the star formation histories of galaxies from z~1 to z~0
- Relation Between Stellar Mass and Star Formation Activity in Galaxies
- The H alpha Galaxy Survey V. The star formation history of late-type galaxies
Cited by in corpus (21)
- Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
- The star formation history of mass-selected galaxies in the COSMOS field
- Galaxy Evolution in Cosmological Simulations With Outflows I: Stellar Masses and Star Formation Rates
- An Older, More Quiescent Universe from Panchromatic SED Fitting of the 3D-HST Survey
- Constraints on star-formation driven galaxy winds from the mass-metallicity relation at z=0
- SDSS IV MaNGA: The global and local stellar mass assemby histories of galaxies
- Reconciling the observed star-forming sequence with the observed stellar mass function
- MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
- The stellar-subhalo mass relation of satellite galaxies
- Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
- The evolution of the star forming sequence in hierarchical galaxy formation models
- The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
- Galaxy downsizing evidenced by hybrid evolutionary tracks
- Cosmological simulations of Milky Way-sized galaxies
- Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
- On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
- Detection of Satellite Remnants in the Galactic Halo with Gaia - II. A modified Great Circle Cell Method
- H-ATLAS/GAMA and HeViCS - Dusty Early-Type Galaxies in Different Environments
- What Regulates Galaxy Evolution? Open Questions in Our Understanding of Galaxy Formation and Evolution
- SED-inferred properties and morphology of Lyman-break galaxies at in the CDF-S