askap continuum surveys of local galaxies michael brown arc future fellow monash university
TRANSCRIPT
Where are we now?
• NVSS / FIRST / SUMMS• 0.5 mJy RMS per beam• 15”-1’ beam
• ~30 uJy RMS per beam in 12 hours Future ASKAP 12
Radio continuum• Continuum detects “hot mode” AGNS.• Continuum can be a good SFR indicator
– Have we been misled by optical colours?– Are SFR indicators properly calibrated?
• ASKAP ADE-12 is great for low z science!– It will detect all* local galaxies (duty cycles, env).– One galaxy per beam and with known locations.– Spectroscopy, morphology, optical, mid-IR
• Done better with completed ASKAP but…
RescalingSpectra
Spectra and H-alpha measurements from Moustakas et al. (2006, 2010) need to be increased by 10%.
Dolley et al. (in prep.)High star-formationLow star-formation
Gal
axy
Clu
ster
ing
Str
engt
h
Projected spatial Scale
Are Red Spirals Forming Stars?
• KAB<10.5 spiral galaxies– Bonne et al. (in prep) and Floyd et al. (sub.)
• NVSS 1.4 GHz as a star formation proxy– 1.4 GHz is not impacted by dust obscuration
• WISE mid-IR to search for warm dust– Dust is heated by star formation
• 21-cm to search for neutral hydrogen– Could star formation resume?
Sample SelectionKAB<10.5T-type > -1NVSS 1.4 GHz coverage228 galaxies
Select galaxies with f1.4 < 2.5 mJy42 galaxies
UV-optical similar to passive E
H-alpha lost in the noise
Spiral arms are blue in UV-optical
IR excess
Red and no NVSS, but Star Forming
Radio continuum• Continuum detects “hot mode” AGNS.• Continuum can be a good SFR indicator
– Have we been misled by optical colours?– Are SFR indicators properly calibrated?
• ASKAP ADE-12 is great for low z science!– It will detect all* local galaxies (duty cycles, env).– One galaxy per beam and with known locations.– Spectroscopy, morphology, optical, mid-IR
• Done better with completed ASKAP but…
Summary• Have we been misled by colour bimodality?• Red spirals are not faded blue spirals.
– Red spirals are brighter than blue spirals (Bonne).• High and low SFR spirals live in similar halos
– The large-scale clustering is similar (Dolley).• Low SFR spirals are not passive spirals
– Infrared excess and PAH emission • Red spirals generally have HI
Infrared SEDsIR excess relative to passive elliptical galaxies
NGC 4725 spectrum shows PAH and dust emission
21-cm
Catalogued HI in redUncatalogued HI in black
228 spirals with KAB < 10.5186 spirals in HI catalogues
42 spirals f1.4 < 2.5 mJy31 spirals in HI catalogues