237 research outputs found
The JCMT Nearby Galaxies Legacy Survey: SCUBA-2 observations of nearby galaxies
We present 850m observations of a sample of 8 nearby spiral galaxies,
made using the SCUBA-2 camera on the James Clerk Maxwell Telescope (JCMT) as
part of the JCMT Nearby Galaxies Legacy Survey (NGLS). We corrected our data
for the presence of the CO line in the SCUBA-2 850m
bandwidth using NGLS HARP data, finding a typical CO contribution of
%. We measured dust column densities, temperatures and opacity indices
by fitting spectral energy distributions constructed from SCUBA-2 and archival
Herschel observations, and used archival GALEX and Spitzer data to make maps of
surface density of star formation (). Typically, comparing
SCUBA-2-derived H surface densities () to gives shallow star formation law indices within galaxies, with
SCUBA-2-derived values typically being sublinear and Herschel-derived values
typically being broadly linear. This difference is likely due to the effects of
atmospheric filtering on the SCUBA-2 data. Comparing the mean values of
and of the galaxies in our sample returns
a steeper star formation law index, broadly consistent with both the
Kennicutt-Schmidt value of 1.4 and linearity. Our results show that a SCUBA-2
detection is a good predictor of star formation. We suggest that Herschel
emission traces gas in regions which will form stars on timescales
Myr, comparable to the star formation timescale traced by GALEX and Spitzer
data, while SCUBA-2 preferentially traces the densest gas within these regions,
which likely forms stars on shorter timescales.Comment: Accepted for publication in MNRAS. 15 pages, 12 figures, 8 tables
(plus 15 pages of appendices, with 31 figures
SCUBA - A submillimetre camera operating on the James Clerk Maxwell Telescope
The Submillimetre Common-User Bolometer Array (SCUBA) is one of a new
generation of cameras designed to operate in the submillimetre waveband. The
instrument has a wide wavelength range covering all the atmospheric
transmission windows between 300 and 2000 microns. In the heart of the
instrument are two arrays of bolometers optimised for the short (350/450
microns) and long (750/850 microns) wavelength ends of the submillimetre
spectrum. The two arrays can be used simultaneously, giving a unique
dual-wavelength capability, and have a 2.3 arc-minute field of view on the sky.
Background-limited performance is achieved by cooling the arrays to below 100
mK. SCUBA has now been in active service for over a year, and has already made
substantial breakthroughs in many areas of astronomy. In this paper we present
an overview of the performance of SCUBA during the commissioning phase on the
James Clerk Maxwell Telescope (JCMT).Comment: 14 pages, 13 figures (1 JPEG), Proc SPIE vol 335
The star-formation law at GMC scales in M33, the Triangulum Galaxy
We present a high spatial resolution study, on scales of 100pc, of the
relationship between star-formation rate (SFR) and gas content within Local
Group galaxy M33. Combining deep SCUBA-2 observations with archival GALEX,
SDSS, WISE, Spitzer and submillimetre Herschel data, we are able to model the
entire SED from UV to sub-mm wavelengths. We calculate the SFR on a
pixel-by-pixel basis using the total infrared luminosity, and find a total SFR
of /yr, somewhat lower than our other two measures
of SFR -- combined FUV and 24m SFR
(/yr) and SED-fitting tool MAGPHYS
(/yr). We trace the total gas using a
combination of the 21cm HI line for atomic hydrogen, and CO(=2-1)
data for molecular hydrogen. We have also traced the total gas using dust
masses. We study the star-formation law in terms of molecular gas, total gas,
and gas from dust. We perform an analysis of the star-formation law on a
variety of pixel scales, from 25 to 500
(100pc to 2kpc). At kpc scales, we find that a linear Schmidt-type power law
index is suitable for molecular gas, but the index appears to be much higher
with total gas, and gas from dust. Whilst we find a strong scale dependence on
the Schmidt index, the gas depletion timescale is invariant with pixel scale.Comment: 19 pages, 15 figures, accepted for publication in MNRA
The Canada-UK Deep Sub-Millimeter Survey II: First identifications, redshifts and implications for galaxy evolution
Identifications are sought for 12 sub-mm sources detected by Eales et al
(1998). Six are securely identified, two have probable identifications and four
remain unidentified with I_AB > 25. Spectroscopic and estimated photometric
redshifts indicate that four of the sources have z < 1, and four have 1 < z <
3, with the remaining four empty field sources probably lying at z > 3. The
spectral energy distributions of the identifications are consistent with those
of high extinction starbursts such as Arp 220. The far-IR luminosities of the
sources at z > 0.5 are of order 3 x 10^12 h_50^-2 L_sun, i.e. slightly larger
than that of Arp 220. Based on this small sample, the cumulative bolometric
luminosity function shows strong evolution to z ~ 1, but weaker or possibly
even negative evolution beyond. The redshift dependence of the far-IR
luminosity density does not appear, at this early stage, to be inconsistent
with that seen in the ultraviolet luminosity density. Assuming that the energy
source in the far-IR is massive stars, the total luminous output from
star-formation in the Universe is probably dominated by the far-IR emission.
The detected systems have individual star-formation rates (exceeding 300
h_50^-2 M_O yr^-1) that are much higher than seen in the ultraviolet selected
samples, and which are sufficient to form substantial stellar populations on
dynamical timescales of 10^8 yr. The association with merger-like morphologies
and the obvious presence of dust makes it attractive to identify these systems
as forming the metal-rich spheroid population, in which case we would infer
that much of this activity has occurred relatively recently, at z ~ 2.Comment: 17 pages text + 14 figures. Accepted for publication in the
Astrophysical Journal. Gzipped tar file contains one text.ps file for text
and tables, one Fig2.jpg file for Fig 2, and 13 Fig*.ps files for the
remaining figure
A Submillimetre Survey of the Hubble Deep Field: Unveiling Dust-Enshrouded Star Formation in the Early Universe
The advent of sensitive sub-mm array cameras now allows a proper census of
dust-enshrouded massive star-formation in very distant galaxies, previously
hidden activity to which even the deepest optical images are insensitive. We
present the deepest sub-mm survey, taken with the SCUBA camera on the James
Clerk Maxwell Telescope (JCMT) and centred on the Hubble Deep Field (HDF). The
high source density on this image implies that the survey is confusion-limited
below a flux density of 2 mJy. However within the central 80 arcsec radius
independent analyses yield 5 reproducible sources with S(850um) > 2 mJy which
simulations indicate can be ascribed to individual galaxies. These data lead to
integral source counts which are completely inconsistent with a no evolution
model, whilst the combined brightness of the 5 most secure sources in our map
is sufficient to account for 30-50% of the previously unresolved sub-mm
background, and statistically the entire background is resolved at about the
0.3 mJy level. Four of the five brightest sources appear to be associated with
galaxies which lie in the redshift range 2 < z < 4. With the caveat that this
is a small sample of sources detected in a small survey area, these submm data
imply a star-formation density over this redshift range that is at least five
times higher than that inferred from the rest-frame ultraviolet output of HDF
galaxies.Comment: to appear in the proceedings of `The Birth of Galaxies', Xth
Rencontres de Blois, 4 pages, 1 postscript figure, uses blois.sty (included
Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
The advent of sensitive sub-mm array cameras now allows a proper census of
dust-enshrouded massive star-formation in very distant galaxies, previously
hidden activity to which even the faintest optical images are insensitive. We
present the deepest sub-mm survey of the sky to date, taken with the SCUBA
camera on the James Clerk Maxwell Telescope and centred on the Hubble Deep
Field. The high source density found in this image implies that the survey is
confusion-limited below a flux density of 2 mJy. However, within the central 80
arcsec radius independent analyses yield 5 reproducible sources with S(850um) >
2 mJy which simulations indicate can be ascribed to individual galaxies. We
give positions and flux densities for these, and furthermore show using
multi-frequency photometric data that the brightest sources in our map lie at
redshifts z~3. These results lead to integral source counts which are
completely inconsistent with a no-evolution model, and imply that massive
star-formation activity continues at redshifts > 2. The combined brightness of
the 5 most secure sources in our map is sufficient to account for 30 - 50% of
the previously unresolved sub-mm background, and we estimate statistically that
the entire background is resolved at about the 0.3 mJy level. Finally we
discuss possible optical identifications and redshift estimates for the
brightest sources. One source appears to be associated with an extreme
starburst galaxy at z~1, whilst the remaining four appear to lie in the
redshift range 2 < z < 4. This implies a star-formation density over this
redshift range that is at least five times higher than that inferred from the
ultraviolet output of HDF galaxies.Comment: 19 pages, 6 figures (to appear as a Nature Article
A high-resolution, dust-selected molecular cloud catalogue of M33, the Triangulum galaxy
We present a catalogue of Giant Molecular Clouds (GMCs) in M33, extracted from cold dust continuum emission. Our GMCs are identified by computing dendrograms. We measure the spatial distribution of these clouds, and characterise their dust properties. Combining these measured properties with CO(J=2–1) and 21cm H i data, we calculate the gas-to-dust ratio (GDR) of these clouds, and from this compute a total cloud mass. In total, we find 165 GMCs with cloud masses in the range of 104-107 M⊙. We find that radially, log10(GDR) = −0.043( ± 0.038) R[kpc] + 1.88( ± 0.15), a much lower GDR than found in the Milky Way, and a correspondingly higher αCO factor. The mass function of these clouds follows a slope proportional to M−2.84, steeper than many previous studies of GMCs in local galaxies, implying that M33 is poorer at forming massive clouds than other nearby spirals. Whilst we can rule out interstellar pressure as the major contributing factor, we are unable to disentangle the relative effects of metallicity and H i velocity dispersion. We find a reasonably featureless number density profile with galactocentric radius, and weak correlations between galactocentric radius and dust temperature/mass. These clouds are reasonably consistent with Larson’s scaling relationships, and many of our sources are co-spatial with earlier CO studies. Massive clouds are identified at large galactocentric radius, unlike in these earlier studies, perhaps indicating a population of CO-dark gas dominated clouds at these larger distances
Multiwaveband Observations of Quasars with Flat Radio Spectra and Strong Millimeter Emission
We present multiwaveband observations of a well selected sample of 28 quasars
and two radio galaxies with flat radio spectra and strong millimeter wave
emission (referred to here as FSRQ's). The observations include multifrequency
VLBI measurements, X-ray observations with ROSAT and submillimeter observations
with the JCMT. Particularly interesting among many findings is a correlation
between the X-ray to millimeter spectral index and fraction of flux density
contained in the VLBI core. This tendency toward higher X-ray fluxes from
sources with stronger jet emission implies that the knots in the jet are the
prominent source of X-rays.Comment: 38 pages, 17 figures, 12 tables, accepted for publication in Ap J
Suppl, May 199
The Canada-UK Deep Submillimetre Survey: First Submillimetre Images, the Source Counts, and Resolution of the Background
We present the first results of a deep unbiased submillimetre survey carried
out at 450 and 850 microns. We detected 12 sources at 850 microns, giving a
surface density of sources with 850-micron flux densities > 2.8mJy of of
0.49+-0.16 per square arcmin. The sources constitute 20-30% of the background
radiation at 850 microns and thus a significant fraction of the entire
background radiation produced by stars. This implies, through the connection
between metallicity and background radiation, that a significant fraction of
all the stars that have ever been formed were formed in objects like those
detected here. The combination of their large contribution to the background
radiation and their extreme bolometric luminosities make these objects
excellent candidates for being proto-ellipticals. Optical astronomers have
recently shown that the UV-luminosity density of the universe increases by a
factor of about 10 between z=0 and z=1 and then decreases again at higher
redshifts. Using the results of a parallel submillimetre survey of the local
universe, we show that both the submillimetre source density and background can
be explained if the submillimetre luminosity density evolves in a similar way
to the UV-luminosity density. Thus, if these sources are ellipticals in the
process of formation, they may be forming at relatively modest redshifts.Comment: 8 pages (LATEX), 6 postscript figures, submitted to ApJ Letter
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