HI mass function optical luminosity function. most baryonic mass in low surface ... HIPASS (HI) remaining fuel star formation future. failed star formation ...
Limits on I.G. HI Clouds: Fisher & Tully 'not cosmologically significant' ... 2000 Zwaan (PhD Thesis) HI Mass Function. 2003 Koribalski/Zwaan ET AL... HIPASS ...
R 17 mag 'NOT' already in one of the official optical target lists for 6dFGS ... Visually matched by 3 people to minimise galaxy selection bias. Results ...
Title: PowerPoint Presentation Author: fbriggs Last modified by: fbriggs Created Date: 11/4/2002 12:53:31 AM Document presentation format: On-screen Show
... Davies, Erwin de Blok, Virginia Kilborn, Suzanne Linder, Karen Masters, Martin ... Low column-density gas in the local Universe. Extragalactic OH Megamaser ...
WALLABY: Local Group Science. Emma Ryan-Weber. Credit: Mario Mateo ... Leo T doesn't fit the idea that reionization surpressed star formation in low ...
Funded year-by-year by the Australian Research Council Linkage Infrastructure ... 'convolve' simulations to compare statistically with observations. ...
High resolution Radio observations. The continuing path to the answer. Supervisor: ... High resolution radio observations needed 216 (5%) Blank Fields ...
Tot. 0. 1/3300. looks like HI is an endangered species !!! Where are the missing baryons ? ... but, only a tiny fraction of total baryons are neutral ...
A New way to Investigating the SFR-Density Relation - HI Galaxy Sample ... Different Investigation of SFR-Density Relation - HI Galaxies Sample to answer the ...
Veronique Buat, Jonathan Davies, Kate Isaak, Walter K Gear, ... R~1000 integrated spectroscopy (Balmer decrement, metallicity...) with CARELEC at the OHP ...
High Velocity Clouds-2 'I've looked at clouds from both sides now ... If HVCs (or CHVCs) are bona fide LG members, they should also exist in other groups. ...
To keep up with next-generation optical/IR telescopes ... Perth. Canberra. Hobart. Adelaide. Melbourne. Sydney. Challenge: Radio frequency interference (RFI) ...
with help from Stuart Wyithe (Melbourne), Martin Zwaan (ESO) ... Halo Occupation Distribution (HOD) modelling. Conditional Luminosity Function (CLF) modelling. ...
What new opportunities flow from the ATCA mm upgrade? mm continuum emission from ... Based on ATCA sensitivity figures, and calculations by Blain et al. (2000) ...
UHECRs: AGNs or Spiral galaxies?... or Ellipticals? with Ghirlanda, Tavecchio, Fraternali, Pareschi MNRAS, 390, L88 Can we discriminate between AGN and spirals?
MORPOLOGICAL & DYNAMICAL PARAMETERS OF HALOS IN VOIDS. Manolis Plionis (NOA ... taking gas into account is under-way using the HR Mare-Nostrum ?CDM Simulations ...
... within 8 Mpc turns out to be 0.10 in units of the global critical density. ... are free from haloes with Vcirc 10km/s any haloes of astronomical interest. ...
CRs from the Moon. Simulated filled aperture. FPA Proposal ... PuMa now gives 8x10 MHz, but PuMa II will give 8x20 MHz ... base-band recording with Puma (II) ...
PAPER (Don Backer) ... Start in 2004 (Don Backer et al.) 100 to 200 MHz. Individual, dual polarization dipoles ... D. Backer. Harvard-Smithsonian: 21cm ...
Tentative evidence that galaxies in high-density regions are redder (see figure) ... Density Ratio Vs B-R for 6dF Galaxy Survey observation -22 dec -42. ...
LAB survey. Bruns et al. 05. Braun & Thilker 04 ... Latest observational (HI) results: ... If in free expansion, mean expansion time 10 Myr, very short. ...
deep Ha, UV imaging of volume-complete 11 Mpc samples - Spitzer followup proposed ... Ha imaging followup of Arecibo ALFALFA HI survey. Fourth Generation: blind ...