38 research outputs found
A multi-transition molecular line study of inward motions towards massive star-forming cores
A multi-transition 3mm molecular line single-pointing and mapping survey
was carried out towards 29 massive star-forming cores in order to search for
the signature of inward motions. Up to seven different transitions, optically
thick lines HCO(1-0), CS(2-1), HNC(1-0), HCN(1-0), CO(1-0) and
optically thin lines CO(1-0), CO(1-0) were observed towards each
source. The normalized velocity differences (V,
V) between the peak velocities of optically thick lines
and optically thin line CO(1-0) for each source were derived. Prominent
inward motions are probably present in either HCO(1-0) or CS(2-1) or
HNC(1-0) observations in most sources. Our observations show that there is a
significant difference in the incidence of blue shifted line asymmetric line
profiles between CS(2-1) and HCO(1-0). The HCO(1-0) shows the highest
occurrence of obvious asymmetric feature, perhaps owing to different optical
depth between CS(2-1) and HCO(1-0). HCO(1-0) appears to be the best
inward motion tracer. The mapping observations of multiple line transitions
enable us to identify six strong infall candidates G123.07-6.31, W75(OH),
S235N, CEP-A, W3(OH), NGC7538. The infall signature is extended up to a linear
scale pc.Comment: 11 pages, 10 figures, 3 tables, accepted for publication in MNRA
The Baryon Oscillation Spectroscopic Survey of SDSS-III
The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the
scale of baryon acoustic oscillations (BAO) in the clustering of matter over a
larger volume than the combined efforts of all previous spectroscopic surveys
of large scale structure. BOSS uses 1.5 million luminous galaxies as faint as
i=19.9 over 10,000 square degrees to measure BAO to redshifts z<0.7.
Observations of neutral hydrogen in the Lyman alpha forest in more than 150,000
quasar spectra (g<22) will constrain BAO over the redshift range 2.15<z<3.5.
Early results from BOSS include the first detection of the large-scale
three-dimensional clustering of the Lyman alpha forest and a strong detection
from the Data Release 9 data set of the BAO in the clustering of massive
galaxies at an effective redshift z = 0.57. We project that BOSS will yield
measurements of the angular diameter distance D_A to an accuracy of 1.0% at
redshifts z=0.3 and z=0.57 and measurements of H(z) to 1.8% and 1.7% at the
same redshifts. Forecasts for Lyman alpha forest constraints predict a
measurement of an overall dilation factor that scales the highly degenerate
D_A(z) and H^{-1}(z) parameters to an accuracy of 1.9% at z~2.5 when the survey
is complete. Here, we provide an overview of the selection of spectroscopic
targets, planning of observations, and analysis of data and data quality of
BOSS.Comment: 49 pages, 16 figures, accepted by A
The Baryon Oscillation Spectroscopic Survey of SDSS-III
The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg(2) to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Ly alpha forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Ly alpha forest and a strong detection from the Data Release 9 data set of the BAO in the clustering of massive galaxies at an effective redshift z = 0.57. We project that BOSS will yield measurements of the angular diameter distance d(A) to an accuracy of 1.0% at redshifts z = 0.3 and z = 0.57 and measurements of H(z) to 1.8% and 1.7% at the same redshifts. Forecasts for Ly alpha forest constraints predict a measurement of an overall dilation factor that scales the highly degenerate D-A(z) and H-1(z) parameters to an accuracy of 1.9% at z similar to 2.5 when the survey is complete. Here, we provide an overview of the selection of spectroscopic targets, planning of observations, and analysis of data and data quality of BOSS