An Anomalous UV Extension in NGC6251

Deep U-band FOC images of the nuclear region of NGC6251 have revealed a region of extended emission which is most probably radiation scattered from a continuum source in the nucleus. This radiation lies interior to a dust ring, is nearly perpendicular to the radio jet axis, and is seen primarily in the FOC U and b filters. The extension has a low observed polarization($\le 10$), and is unlikely to arise from line emission. We know of no other examples similar to what we have found in NGC 6251, and we offer some tentative explanations. The nuclear morphology shows clear similarities to that seen in the nucleus of NGC 4261 except for the extended U-band radiation.Comment: 14 pages AAStex format + 4 figures; accepted for publication in ApJ Letter

Response to Comment on `Undamped electrostatic plasma waves' [Phys. Plasmas 19, 092103 (2012)]

Numerical and experimental evidence is given for the occurrence of the plateau states and concomitant corner modes proposed in \cite{valentini12}. It is argued that these states provide a better description of reality for small amplitude off-dispersion disturbances than the conventional Bernstein-Greene-Kruskal or cnoidal states such as those proposed in \cite{comment

The First CO Map of a Low Surface Brightness Galaxy

Using the Owens Valley Radio Observatory Millimeter-Wavelength Array (OVRO) we have obtained the first CO map of a low surface brightness (LSB) galaxy. The studied galaxy, UGC 01922, was chosen for these observations because both of its previous CO detection with the IRAM 30m telescope and its classification as a Malin 1 `cousin' - an LSB galaxy with M_HI > 10^10 Msol. The OVRO map detected approximately 65% of the CO(1-0) flux found earlier with the single dish measurements, giving a detected gas mass equivalent to M_H2 = 1.1X10^9 Msol. The integrated gas peak lies at the center of the galaxy and coincides with both the optical and 1.4 GHz continuum emission peaks. The molecular gas extends well beyond the OVRO beam size (~4'' or 3 kpc), covering ~25% of the optical bulge. In all, perhaps the most remarkable aspect of this map is its unexceptional appearance. Given that it took over ten years to successfully detect molecular gas in any low surface brightness system, it is surprising that the appearance and distribution of UGC 01922's CO is similar to what would be expected for a high surface brightness galaxy in the same morphological class.Comment: 5 pages, including 3 figures and 3 tables. also available online at http://www.gb.nrao.edu/~koneil. Accepted by ApJ

Undamped electrostatic plasma waves

Electrostatic waves in a collision-free unmagnetized plasma of electrons with fixed ions are investigated for electron equilibrium velocity distribution functions that deviate slightly from Maxwellian. Of interest are undamped waves that are the small amplitude limit of nonlinear excitations, such as electron acoustic waves (EAWs). A deviation consisting of a small plateau, a region with zero velocity derivative over a width that is a very small fraction of the electron thermal speed, is shown to give rise to new undamped modes, which here are named {\it corner modes}. The presence of the plateau turns off Landau damping and allows oscillations with phase speeds within the plateau. These undamped waves are obtained in a wide region of the $(k,\omega_{_R})$ plane ($\omega_{_R}$ being the real part of the wave frequency and $k$ the wavenumber), away from the well-known `thumb curve' for Langmuir waves and EAWs based on the Maxwellian. Results of nonlinear Vlasov-Poisson simulations that corroborate the existence of these modes are described. It is also shown that deviations caused by fattening the tail of the distribution shift roots off of the thumb curve toward lower $k$-values and chopping the tail shifts them toward higher $k$-values. In addition, a rule of thumb is obtained for assessing how the existence of a plateau shifts roots off of the thumb curve. Suggestions are made for interpreting experimental observations of electrostatic waves, such as recent ones in nonneutral plasmas.Comment: 11 pages, 10 figure

Where are the Baryons?

New, high resolution, large-scale, cosmological hydrodynamic galaxy formation simulations of a standard cold dark matter model (with a cosmological constant) are utilized to predict the distribution of baryons at the present and at moderate redshift. It is found that the average temperature of baryons is an increasing function of time, with most of the baryons at the present time having a temperature in the range 10^{5-7} K. Thus, not only is the universe dominated by dark matter, but more than one half of the normal matter is yet to be detected. Detection of this warm/hot gas poses an observational challenge, requiring sensitive EUV and X-ray satellites. Signatures include a soft, cosmic X-ray background, apparent warm components in hot clusters due to both intrinsic warm intra-cluster gas and warm inter-cluster gas projected onto clusters along the line of sight, absorption lines in X-ray and UV quasar spectra [e.g., O VI (1032,1038)A lines, OVII 574 eV line], strong emission lines (e.g., O VIII 653 eV line) and low redshift, broad, low column density \lya absorption lines. We estimate that approximately 1/4 of the extragalactic soft X-ray background (SXRB) (at 0.7 keV) arises from the warm/hot gas, half of it coming from $z<0.65$ and three-quarters from $z<1.00$, so the source regions should be identifiable on deep optical images.Comment: ApJ in press, revised (fig 3 is in jpg). Whole paper including fig3.ps can be obtained at "http://astro.princeton.edu/~cen/PAPERS_TO_APPEAR/64

Nonlinear saturation of electrostatic waves: mobile ions modify trapping scaling

The amplitude equation for an unstable electrostatic wave in a multi-species Vlasov plasma has been derived. The dynamics of the mode amplitude $\rho(t)$ is studied using an expansion in $\rho$; in particular, in the limit $\gamma\rightarrow0^+$, the singularities in the expansion coefficients are analyzed to predict the asymptotic dependence of the electric field on the linear growth rate $\gamma$. Generically $|E_k|\sim \gamma^{5/2}$, as $\gamma\rightarrow0^+$, but in the limit of infinite ion mass or for instabilities in reflection-symmetric systems due to real eigenvalues the more familiar trapping scaling $|E_k|\sim \gamma^{2}$ is predicted.Comment: 13 pages (Latex/RevTex), 4 postscript encapsulated figures which are included using the utility "uufiles". They should be automatically included with the text when it is downloaded. Figures also available in hard copy from the authors ([email protected]

Ion exchange trap and release of [C-11]CO2

Introduction Recently in our laboratory we needed a reliable and relatively simple source of aqueous solutions of [11C]CO2. We examined various methods of trapping [11C]CO2 gas both in solution and on ion exchange resins, followed by elution into aqueous phase. We favor simple methods that have high trapping and elution efficiencies and produce a highly concentrated solution. Furthermore, we desired methods that would minimize the use of hazardous reagents and materials with respect to both handling and disposal. We also considered the formulation of the final solution in terms of chemical compatibility with contacted materials, working with the assumption that dilute bicarbonate or carbonate solutions will have little reactivity with many materials. In a phantom, compatibility with materials (i.e. plastics, glues, metals, etc.) is important (1-4), while in (bio)geochemical studies – where transport of carbon is important – the chemical form of the radiolabelled molecule is important, but compatibility must be determined on a case-by-case basis (5-7). Small medical cyclotrons can easily produce carbon-11 as gaseous [11C]CO2, and various methods are utilized to incorporate carbon-11 into solution, often with unfavorable resource requirements, costs, or chemical properties. Commonly [11C]CO2 gas is bubbled through a strong base, forming the carbonate anion; but neutralizing a strong base (as to avoid special handling or disposal requirements) requires a large volume of diluent or buffer; or a very precise addition of acid – which if done improperly – may lead to an acidic pH and subsequent loss of [11C]CO2 from solution (8,9). Alternatively, [11C]CO2 (or [11C]CH4) can be converted to [11C]CH3I at high-yield, but requires specialized, expensive radio-synthesis equipment (10-12). [11C]CH3I can then be trapped in DMSO (albeit providing a volatile and hazardous solution) or used as a synthon en route to water soluble compounds such as [11C]choline (13). Finally, leftover radiolabelled radiopharmaceuticals from a carbon-11 imaging experiment could be used, but chemical compatibility (i.e. lipophilicity) of the radiolabelled compound may be of concern. Carbon dioxide gas will dissolve with a solubility of 1.5 g/L at STP (9) and slowly react with water to generate carbonic acid (H2CO3), a weak acid. Passing [11C]CO2 through a base-activated ion exchange cartridge, the [11C]CO2 reacts with hydroxide ions to form [11C]carbonate which is bound to the resin due to its higher selectivity for carbonate than hydroxide (14). Elution with excess bicarbonate displaces [11C]carbonate and neutralizes any remaining hydroxide, providing a 11C aqueous solution that is mildly basic, chemically non-hazardous, and very concentrated. Material and Methods [11C]CO2 gas trapping efficiency was evaluated for solutions and base-activated ion exchange resins. The gas was delivered either rapidly in a high-flow bolus directly from the cyclotron target or slowly in a low-flow helium stream during heating of a carbosieves column. Elution efficiency of ion exchange cartridges were evaluated for both fraction of trapped activity eluted and volume of solution needed for elution. [11C]CO2 was produced via the 14N(p,α)11C reaction on a CTI RDS111 – 11 MeV cyclotron at the Lawrence Berkeley National Laboratory’s Bio-medical Isotope Facility. The 7 mL target is pressurized to 315 psi with 1% O2/N2 gas, equating to 150 mL gas at STP. For direct-from-target trapping experiments, the target was decompressed and routed to the cartridge via 50 feet of 0.020” I.D. tubing until the target falls to atmospheric pressure (~55 seconds) providing an inhomogeneous flow – a short rapid burst of flow followed by a longer low-flow bleed. For helium-eluted experiments, the [11C]CO2 was unloaded from the cyclotron target and trapped on a room-temperature carbosieves column (15). Target gases were subsequently flushed from the column for 30 seconds with helium at 50 mL/min. After heating the column to 125 °C without gas flow, [11C]CO2 was eluted off the column in helium at 15 mL/min. [11C]CO2/He was bubbled through 9 aqueous and 2 organic solutions to test for trapping efficiency in a slow, steady helium stream at 15 mL/min (sodium hydroxide (0.96M, 0.096M, 0.0096M), sodium bicarbonate (1.14M, 0.57M, 0.057M), sodium carbonate (2.0M, 1.0M, 0.10M), ethanol, and DMSO (2mL ea.). An Ascarite-filled cartridge was attached to trap any untrapped [11C]CO2. Measures of radioactivity were made using a Capintec CRC-15R dose calibrator. Trapping efficiency for solutions is calculated as the fraction of radioactivity captured in solution relative to the sum of the solution and the Ascarite trap. Three different commercially available, ion ex-change cartridges were evaluated for trapping and elution efficiencies. FIGURE 1 shows a photo-graphic comparison of the physical size and shapes of the cartridges as well as a X-ray computed tomography (CT) cross sectional view of the internal ion exchange resin volume and dead volume of the cartridges. All cartridges were activated with 1 mL of 1 N aqueous NaOH followed by passing 10 mL deionized water then 10 mL of air through the cartridge. In both direct-from-target (n = 4) and helium-stream experiments (n = 3 or 4), cartridges were connected to [11C]CO2 delivery lines via Luer connections. The gas exiting the cartridge passed through an empty 3 mL crimp-top vial as a liquid trap en route to an Ascarite trap on the vent needle as described above. Trapping efficiency for cartridges is calculated as the fraction of radioactivity captured on the cartridge relative to the sum of the cartridge, the empty vial, and the Ascarite trap. Cartridges were eluted with 0.5 mL of saturated sodium bicarbonate solution (1.14 M @ 20°C) followed by 9.5 mL water and 10 mL air. Elution efficiency is calculated as the fraction of radioactivity eluted in 10 mL relative to the sum of the spent cartridge following elution and the 10 mL eluate (Equation 5). The pH of the eluate was measured using 0-14 pH test strips. Results and Conclusion The trapping of [11C]CO2 in all solutions was less than 70% of the total radioactivity with the exception of the 0.96 M and 0.096 M NaOH. With a higher concentration of base driving equilibrium towards carbonate stability, it could be expected that the most basic solution had the best trapping efficiency, but this attribute also means it is least desirable solution to work with from a hazardous material or chemical compatibility perspective. When [11C]CO2 was delivered in a helium stream, all three cartridges performed at near 100% efficiency, as shown in FIGURE 4. With higher flow, direct-from-target delivery, the cartridges trapped [11C]CO2 with a wider range of efficiencies: ICOH (99 ± 1 %), ORTG (90 ± 2 %), and QMA (79 ± 4 %). Elution resulted in > 99 % release of carbon-11 activity for both QMA and ORTG cartridges, but only 39 ± 3 % release from the ICOH cartridge. Elution efficiency of the trapped radioactivity (Equation 5) was independent of the method of [11C]CO2 delivery. Across all cartridges and delivery methods, the eluate was at about pH = 10. We recommend that the ORTG cartridge be used for trapping of [11C]CO2 gas with elution by > 300 µL of saturated bicarbonate solution. This recommendation is based on the better trapping for ORTG cartridges compared to the QMA cartridges in the direct-from-target [11C]CO2 delivery method and the smaller volume needed for elution of all trapped carbon. This method excels based on its simplicity, adaptability to automation, low-cost ($5/cartridge), and observations that a single ORTG cartridge suffers no loss of performance after multiple uses. A potential disadvantage to this method is that it involves using a carbon-containing eluent, which means that this method cannot be used for imaging experiments that require high specific activity. However, considering the eluate is a mildly basic aqueous solution, we expect that it will be compatible with a wide variety of materials and experimental applications

The Energy of a Plasma in the Classical Limit

When \lambda_{T} << d_{T}, where \lambda_{T} is the de Broglie wavelength and d_{T}, the distance of closest approach of thermal electrons, a classical analysis of the energy of a plasma can be made. In all the classical analysis made until now, it was assumed that the frequency of the fluctuations \omega << T (k_{B}=\hbar=1). Using the fluctuation-dissipation theorem, we evaluate the energy of a plasma, allowing the frequency of the fluctuations to be arbitrary. We find that the energy density is appreciably larger than previously thought for many interesting plasmas, such as the plasma of the Universe before the recombination era.Comment: 10 pages, 2 figures, accepted for publication in Phys.Rev.Let