10,975 research outputs found
Recommended from our members
Millimetre and submillimetre molecular line observations of the reflection nebula NGC 2023
Observations in the CO J = 2 - 1, CO J = 3 - 2 and HCO+ J = 4 - 3 transitions of the molecular cloud associated with NGC 2023 are presented. The observations reveal the complex structure of the gas in the surrounding cloud, and show the presence of several hot-spots which may represent separate bodies of gas. A search has been made for the source of excitation of two nearby groups of Herbig-Haro objects recently discovered by Malin et al. (1987). No such objects can be clearly identified from the data. CO J = 3 - 2 spectra taken at positions lying on the CO J = 1 - 0 shell observed by Gatley et al. (1987) show marked enhancements in peak line strength relative to coincident CO J = 2 - 1 data. By contrast, no such enhancements are observed away from the shell. Observations of the submillimeter wavelength HCO+ J = 4 - 3 transition show that the line strength is greatest in the vicinity of the shell structure. Simple large velocity gradient modeling of the excitation conditions of the shell material suggests that the gas may be hot (Tkin ~ 140 K), dense, and optically thin
Real Space Approach to CMB deboosting
The effect of our Galaxy's motion through the Cosmic Microwave Background
rest frame, which aberrates and Doppler shifts incoming photons measured by
current CMB experiments, has been shown to produce mode-mixing in the multipole
space temperature coefficients. However, multipole space determinations are
subject to many difficulties, and a real-space analysis can provide a
straightforward alternative. In this work we describe a numerical method for
removing Lorentz- boost effects from real-space temperature maps. We show that
to deboost a map so that one can accurately extract the temperature power
spectrum requires calculating the boost kernel at a finer pixelization than one
might naively expect. In idealized cases that allow for easy comparison to
analytic results, we have confirmed that there is indeed mode mixing among the
spherical harmonic coefficients of the temperature. We find that using a boost
kernel calculated at Nside=8192 leads to a 1% bias in the binned boosted power
spectrum at l~2000, while individual Cls exhibit ~5% fluctuations around the
binned average. However, this bias is dominated by pixelization effects and not
the aberration and Doppler shift of CMB photons that causes the fluctuations.
Performing analysis on maps with galactic cuts does not induce any additional
error in the boosted, binned power spectra over the full sky analysis. For
multipoles that are free of resolution effects, there is no detectable
deviation between the binned boosted and unboosted spectra. This result arises
because the power spectrum is a slowly varying function of and does not show
that, in general, Lorentz boosts can be neglected for other cosmological
quantities such as polarization maps or higher-point functions.Comment: 8 pages, submitted to MNRA
Recommended from our members
A submillimetre wavelength spectral line search of the Orion molecular cloud core
A submillimetre wavelength molecular line search of the Orion molecular cloud has been made covering a total of about 5 percent of the frequency range 342.8 - 358.6 GHz. This search, coupled with the authors' previous observations of submillimetre transitions in this cloud, has led to the detection of 22 transitions of 14 molecular species, of which 16 are reported here for the first time. No unidentified lines have been detected in the present search. Mapping observations have been obtained for several of the lines and, in the case of H2CO the authors have been able to compare the present data with that obtained from other telescopes, to estimate the density and abundance in the emitting region
Multidimensional spectroscopy with a single broadband phase-shaped laser pulse
We calculate the frequency-dispersed nonlinear transmission signal of a
phase-shaped visible pulse to fourth order in the field. Two phase profiles, a
phase-step and phase-pulse, are considered. Two dimensional signals obtained by
varying the detected frequency and phase parameters are presented for a three
electronic band model system. We demonstrate how two-photon and stimulated
Raman resonances can be manipulated by the phase profile and sign, and selected
quantum pathways can be suppressed.Comment: 26 pages, 15 figure
NICMOS Observations of the Pre-Main-Sequence Planetary Debris System HD 98800
Spectral energy distributions (SEDs) from 0.4 to 4.7 microns are presented
for the two principal stellar components of HD~98800, A and B. The third major
component, an extensive planetary debris system (PDS), emits > 20% of the
luminosity of star B in a blackbody SED at 164 +/- 5K extending from mid-IR to
millimeter-wavelengths. At 0.95 microns a preliminary upper limit of < 0.06 is
obtained for the ratio of reflected light to the total from star B. This result
limits the albedo of the PDS to < 0.3. Values are presented for the
temperature, luminosity, and radius of each major systemic component.
Remarkable similarities are found between the PDS and the interplanetary debris
system around the Sun as it could have appeared a few million years after its
formation.Comment: LaTeX, 9 pages with 1 encapsulated postscript figure and one
specially formatted Table which is rendered as a postscript file and included
as a figure. Accepted for publication in Astrophysical Journal Letter
Recommended from our members
A 257-273 GHz spectral survey of the OMC1 cloud core
A spectral line survey of the OMC1 cloud core has been obtained, over the frequency range 257.04-273.02 GHz, using the James Clerk Maxwell 15-m submillimeter telescope. Additional observations have been made centered at 229.4, 231.2, 237.3, and 239.1 GHz. A new algorithm was used to deconvolve the original double-sideband data, and its performance is critically discussed.
181 distinct spectral lines were detected, ~ 7 of which are not identifiable with known molecular transitions. Between 18 and 21 molecular species were detected, including up to 10 isotopically-substituted forms. The line strengths are greater by a factor of 1.9 (on average) than in an earlier OVRO survey orf similar frequencies, made using a larger beam. The current results therefore provide a substantial data base of typical line strengths for future high-resolution studies of the OMC1 core
Search for Inclusive b → sl^+l^-
We have searched for the effective flavor changing neutral-current decays b→sl^+l^- using an inclusive method. We set upper limits on the branching ratios B(b→se^+e^-)<5.7×10^(-5), B(b→sμ^+μ^-)<5.8×10^(-5), and B(b→se^±μ^∓)<2.2×10^(-5) [at 90% confidence level (C.L.)]. Combing the dielectron and dimuon decay modes we find B(b→sl^+l^-)<4.2×10^(-5) (at 90% C.L.)
Promoting Physical Activity in Low Income African Americans: Project LAPS
Low income African Americans are at increased risk for physical inactivity and related chronic illnesses. Thus, effective interventions are needed to address these health disparities. The current study examined the efficacy of a home-based physical activity intervention among a low income African American sample with high rates of chronic illnesses (obesity, hypertension, diabetes, high cholesterol). Participants (n=214) were randomly assigned to either the home-based physical activity intervention (self-help print materials, five monthly newsletters, two telephone counseling sessions) or an attention control condition, which promoted healthy diet. Results indicated that the intervention did not produce significantly greater increases in physical activity from baseline to six months than the control group. Lessons learned from the current study include the importance of using proactive retention strategies with low income African American participants and taking into consideration the cultural relevance of the intervention
- …