1,130 research outputs found
Detection of SiO emission from a massive dense cold core
We report the detection of the SiO (J = 2 - 1) transition from the massive
cold dense core G333.125-0.562. The core remains undetected at wavelengths
shorter than 70 micron and has compact 1.2 mm dust continuum. The SiO emission
is localised to the core. The observations are part of a continuing
multi-molecular line survey of the giant molecular cloud G333. Other detected
molecules in the core include 13CO, C18O, CS, HCO+, HCN, HNC, CH3OH, N2H+, SO,
HC3N, NH3, and some of their isotopes. In addition, from NH3 (1,1) and (2,2)
inversion lines, we obtain a temperature of 13 K. From fitting to the spectral
energy distribution we obtain a colour temperature of 18 K and a gas mass of 2
x 10^3 solar mass. We have also detected a 22 GHz water maser in the core,
together with methanol maser emission, suggesting the core will host massive
star formation. We hypothesise that the SiO emission arises from shocks
associated with an outflow in the cold core.Comment: 6 pages, 4 figures, 1 table, to be published in MNRA
Solution of the symmetric eigenproblem AX=lambda BX by delayed division
Delayed division is an iterative method for solving the linear eigenvalue problem AX = lambda BX for a limited number of small eigenvalues and their corresponding eigenvectors. The distinctive feature of the method is the reduction of the problem to an approximate triangular form by systematically dropping quadratic terms in the eigenvalue lambda. The report describes the pivoting strategy in the reduction and the method for preserving symmetry in submatrices at each reduction step. Along with the approximate triangular reduction, the report extends some techniques used in the method of inverse subspace iteration. Examples are included for problems of varying complexity
Anomalous Thermoelectric power of over-doped Bi2Sr2CaCu2O8 superconductor
Temperature dependence of thermoelectric power S(T) of three differently
processed Bi2Sr2CaCu2O8 (Bi2212) samples, viz. as-processed melt quenched
(Bi2212-MQ), 6000C N2-annealed (Bi2212-N2) and 6000C O2-annealed (Bi2212-O2) is
reported here. All the samples possess single-phase character and their
superconducting transition temperatures (TcR=0) are 85 K, 90 K and 72 K
respectively for Bi2212-MQ, Bi2212-N2 and Bi2212-O2. While Bi2212-MQ and
Bi2212-N2 samples are in near optimum doping regime, Bi2212-O2 is an over-doped
sample. TcS=0 values obtained through S(T) data are also in line with those
deduced from the temperature dependence of resistance and DC magnetization.
Interestingly, S(T) behaviour of the optimally-doped Bi2212-MQ and Bi2212-N2
samples is seen to be positive in whole temperature range, it is found negative
for the over-doped Bi2212-O2 sample above TcS=0. These results have been seen
in the light of the recent band structure calculations and the ensuing split
Fermi surface as determined by angle-resolved photoelectron spectroscopy
(ARPES).Comment: 11 Pages Text + Figs: comments welcome ([email protected]
Observations and radiative transfer modelling of a massive dense cold core in G333
Cold massive cores are one of the earliest manifestations of high mass star
formation. Following the detection of SiO emission from G333.125-0.562, a cold
massive core, further investigations of the physics, chemistry and dynamics of
this object has been carried out. Mopra and NANTEN2 molecular line profile
observations, Australia Telescope Compact Array (ATCA) line and continuum
emission maps, and Spitzer 24 and 70 \mum images were obtained. These new data
further constrain the properties of this prime example of the very early stages
of high mass star formation. A model for the source was constructed and
compared directly with the molecular line data using a 3D molecular line
transfer code - MOLLIE. The ATCA data reveal that G333.125-0.562 is composed of
two sources. One of the sources is responsible for the previously detected
molecular outflow and is detected in the Spitzer 24 and 70 \mum band data.
Turbulent velocity widths are lower than other more active regions of G333
which reflects the younger evolutionary stage and/or lower mass of this core.
The molecular line modelling requires abundances of the CO isotopes that
strongly imply heavy depletion due to freeze-out of this species onto dust
grains. The principal cloud is cold, moderately turbulent and possesses an
outflow which indicates the presence of a central driving source. The secondary
source could be an even less evolved object as no apparent associations with
continuum emissions at (far-)infrared wavelengths.Comment: 10 pages, accepted to MNRA
On expansion parallax distances for planetary nebulae
The distances to individual wind-driven bubbles such as Planetary Nebulae
(PNe) can be determined using expansion parallaxes: the angular expansion
velocity in the sky is compared to the radial velocity of gas measured
spectroscopically. Since the one is a pattern velocity, and the other a matter
velocity, these are not necessarily the same. Using the jump conditions for
both shocks and ionization fronts, I show that for typical PNe the pattern
velocity is 20 to 30% larger than the material velocity, and the derived
distances are therefore typically 20 to 30% too low. I present some corrected
distances and suggest approaches to be used when deriving distances using
expansion parallaxesComment: 7 pages, 6 figures, accepted for publication in A&
Analysis of MAGSAT data of the Indian region
Progress in the development of software for reading MAGSAT data tapes and for the reduction of anomaly data, and in the preparation of data for magnetic anomaly maps is reported
Radio continuum properties of young planetary nebulae
We have selected a small sample of post-AGB stars in transition towards the
planetary nebula and present new Very Large Array multi-frequency high-angular
resolution radio observations of them. The multi-frequency data are used to
create and model the targets' radio continuum spectra, proving that these stars
started their evolution as very young planetary nebulae. In the optically thin
range, the slopes are compatible with the expected spectral index (-0.1). Two
targets (IRAS 18062+2410 and 17423-1755) seem to be optically thick even at
high frequency, as observed in a handful of other post-AGB stars in the
literature, while a third one (IRAS 20462+3416) shows a possible contribution
from cold dust. In IRAS 18062+2410, where we have three observations spanning a
period of four years, we detect an increase in its flux density, similar to
that observed in CRL 618.
High-angular resolution imaging shows bipolar structures that may be due to
circumstellar tori, although a different hypothesis (i.e., jets) could also
explain the observations. Further observations and monitoring of these sources
will enable us to test the current evolutionary models of planetary nebulae.Comment: 8 pages, 3 figures, accepted for publication in MNRA
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