Mass Loss From Planetary Nebulae in Elliptical Galaxies

Early-type galaxies possess a dilute hot (2-10E6 K) gas that is probably the thermalized ejecta of the mass loss from evolving stars. We investigate the processes by which the mass loss from orbiting stars interacts with the stationary hot gas for the case of the mass ejected in a planetary nebula event. Numerical hydrodynamic simulations show that at first, the ejecta expands nearly symmetrically, with an upstream bow shock in the hot ambient gas. At later times, the flow past the ejecta creates fluid instabilities that cause about half of the ejecta to separate and the other half to flow more slowly downstream in a narrow wake. When radiative cooling is included, most of the material in the wake (>80%) remains below 1E5 K while the separated ejecta is hotter (1E5-1E6 K). The separated ejecta is still less than one-quarter the temperature of the ambient medium and the only way it will reach the temperature of the ambient medium is through turbulent mixing (after the material has left the grid). These calculations suggest that a significant fraction of the planetary nebula ejecta may not become part of the hot ambient material. This is in contrast to our previous calculations for continuous mass loss from giant stars in which most of the mass loss became hot gas. We speculate that detectable OVI emission may be produced, but more sophisticated calculations will be required to determine the emission spectrum and to better define the fraction of cooled material.Comment: 34 pages with 20 figures. Higher quality figures are in the ApJ versio

Six-year mortality in a street-recruited cohort of homeless youth in San Francisco, California.

Objectives. The mortality rate of a street-recruited homeless youth cohort in the United States has not yet been reported. We examined the six-year mortality rate for a cohort of street youth recruited from San Francisco street venues in 2004. Methods. Using data collected from a longitudinal, venue-based sample of street youth 15-24 years of age, we calculated age, race, and gender-adjusted mortality rates. Results. Of a sample of 218 participants, 11 died from enrollment in 2004 to December 31, 2010. The majority of deaths were due to suicide and/or substance abuse. The death rate was 9.6 deaths per hundred thousand person-years. The age, race and gender-adjusted standardized mortality ratio was 10.6 (95% CI [5.3-18.9]). Gender specific SMRs were 16.1 (95% CI [3.3-47.1]) for females and 9.4 (95% CI [4.0-18.4]) for males. Conclusions. Street-recruited homeless youth in San Francisco experience a mortality rate in excess of ten times that of the states general youth population. Services and programs, particularly housing, mental health and substance abuse interventions, are urgently needed to prevent premature mortality in this vulnerable population

Nonlocal boundary conditions for corrugated acoustic metasurface with strong near field interactions

The propagation of long-wavelength sound in the presence of a metasurface made by arranging acoustic resonators periodically upon or slightly above an impervious substrate is studied. The method of two-scale asymptotic homogenization is used to derive effective boundary conditions, which account for both the surface corrugation and the low-frequency resonance. This method is applied to periodic arrays of resonators of any shape operating in the long-wavelength regime. The approach relies on the existence of a locally periodic boundary layer developed in the vicinity of the metasurface, where strong near-field interactions of the resonators with each other and with the substrate take place. These local effects give rise to an effective surface admittance supplemented by nonlocal contributions from the simple and double gradients of the pressure at the surface. These phenomena are illustrated for the periodic array of cylindrical Helmholtz resonators with an extended inner duct. Effects of the centre-to-centre spacing and orientation of the resonators' opening on the nonlocality and apparent resonance frequency are studied. The model could be used to design metasurfaces with specific effective boundary conditions required for particular applications

X-ray Isophotes in a Rapidly Rotating Elliptical Galaxy: Evidence of Inflowing Gas

We describe two-dimensional gasdynamical computations of the X-ray emitting gas in the rotating elliptical galaxy NGC 4649 that indicate an inflow of about one solar mass per year at every radius. Such a large instantaneous inflow cannot have persisted over a Hubble time. The central constant-entropy temperature peak recently observed in the innermost 150 parsecs is explained by compressive heating as gas flows toward the central massive black hole. Since the cooling time of this gas is only a few million years, NGC 4649 provides the most acutely concentrated known example of the cooling flow problem in which the time-integrated apparent mass that has flowed into the galactic core exceeds the total mass observed there. This paradox can be resolved by intermittent outflows of energy or mass driven by accretion energy released near the black hole. Inflowing gas is also required at intermediate kpc radii to explain the ellipticity of X-ray isophotes due to spin-up by mass ejected by stars that rotate with the galaxy and to explain local density and temperature profiles. We provide evidence that many luminous elliptical galaxies undergo similar inflow spin-up. A small turbulent viscosity is required in NGC 4649 to avoid forming large X-ray luminous disks that are not observed, but the turbulent pressure is small and does not interfere with mass determinations that assume hydrostatic equilibrium.Comment: 21 pages, 9 figures, accepted for publication by Ap

The Cool ISM in Elliptical Galaxies. II. Gas Content in the Volume - Limited Sample and Results from the Combined Elliptical and Lenticular Surveys

We report new observations of atomic and molecular gas in a volume limited sample of elliptical galaxies. Combining the elliptical sample with an earlier and similar lenticular one, we show that cool gas detection rates are very similar among low luminosity E and SO galaxies but are much higher among luminous S0s. Using the combined sample we revisit the correlation between cool gas mass and blue luminosity which emerged from our lenticular survey, finding strong support for previous claims that the molecular gas in ellipticals and lenticulars has different origins. Unexpectedly, however, and contrary to earlier claims, the same is not true for atomic gas. We speculate that both the AGN feedback and merger paradigms might offer explanations for differences in detection rates, and might also point towards an understanding of why the two gas phases could follow different evolutionary paths in Es and S0s. Finally we present a new and puzzling discovery concerning the global mix of atomic and molecular gas in early type galaxies. Atomic gas comprises a greater fraction of the cool ISM in more gas rich galaxies, a trend which can be plausibly explained. The puzzle is that galaxies tend to cluster around molecular-to-atomic gas mass ratios near either 0.05 or 0.5.Comment: 37 pages, including 4 tables and 12 figures. Accepted for publication in the Astrophysical Journa

On the Number of Comets Around White Dwarf Stars: Orbit Survival During the Late Stages of Stellar Evolution

The accretion of comets onto DA white dwarfs can produce observable metal absorption lines. We show here that comet systems around the progenitor main sequence star are vulnerable to being lost during asymptotic giant branch mass loss, if the mass loss is sufficiently asymmetric to impart modest linear momentum to the white dwarf. This may have bearing on the frequency of observation of heavy elements in white dwarf stars, and on inferences regarding the frequency of comet systems, if the imparted linear velocities of white dwarfs can be estimated.Comment: 19 pages, 8 figures, AASTeX-4.0, to be published in ApJ (7/1/98); replaced with slight modifications to intro text and reference

The Development and In Vivo Immunologic Assessment of Biodegradable Microparticles Incorporating CPDI-02 and Mucosal Protein Vaccine

Encapsulation in biodegradable microparticles (MPs) is a promising approach to increase the efficacy of intranasally administered protein vaccines. The generation of long-lived adaptive immune responses against encapsulated protein vaccines, however, requires the incorporation of a suitable mucosal adjuvant. CPDI-02—a complement peptide-derived immunostimulant that selectively activates dendritic cells and macrophages over neutrophils while minimizing the inflammatory side effects of parent C5a—has previously been incorporated into both systemic and mucosal vaccine formulations via direct conjugation to chemical moieties, peptides, proteins, inactivated pathogens, and the surface of biodegradable particles, to enhance Th1-biased cellular immune responses. The effect of CPDI-02 surface conjugation to MPs encapsulating protein vaccine on short- and long-term mucosal and systemic humoral immune responses, however, has not previously been assessed. Further, alternative strategies for incorporating CPDI-02 into PLGA particles encapsulating protein vaccine (such as co-encapsulation of CPDI-02 with protein vaccine; or separately encapsulating protein vaccine and CPDI-02 and co-administering) have not been explored. In this dissertation, we report that respiratory immunization of naive mice with the model antigen ovalbumin (OVA) encapsulated in PLGA MP surface-conjugated with CPDI-02 generated: (i) increased numbers of OVA-specific IgA, IgM, and IgG antibody secreting cells (ASCs) in the lungs and spleen, (ii) increased short- and long-lived mucosal IgA and IgG antibody titers, and (iii) increased short- and long-lived OVA-specific serum titers of IgG subclasses relative to encapsulation in particles modified with scrambled, inactivated CPDI-02 and PBS vehicle control. We further report that co-administration of CPDI-02 and OVA separately encapsulated in PLGA MPs via the intranasal route increases the generation of: (i) short-term OVA-specific IgA ASCs in the lungs, (ii) mucosal IgA and IgG antibody titers, (iii) OVA-specific IgG ASCs in the spleen, (iv) OVA-specific serum titers of IgG subclasses, and (v) OVA-specific CD4+ and CD8+ T cells in the spleen, compared to other strategies for incorporating CPDI-02 into MPs encapsulating protein vaccine. Thus, the strategy by which CPDI-02 is incorporated into MPs affects the generation of mucosal and systemic cellular and humoral immune responses by encapsulated protein vaccines after respiratory immunization

Oxygen Metallicity Determinations from Optical Emission Lines in Early-type Galaxies

We measured the oxygen abundances of the warm (T$\sim 10^{4}K$) phase of gas in seven early-type galaxies through long-slit observations. A template spectra was constructed from galaxies void of warm gas and subtracted from the emission-line galaxies, allowing for a clean measurement of the nebular lines. The ratios of the emission lines are consistent with photoionization, which likely originates from the UV flux of post-asymototic giant branch (PAGB) stars. We employ H II region photoionization models to determine a mean oxygen metallicity of $1.01\pm0.50$ solar for the warm interstellar medium (ISM) in this sample. This warm ISM 0.5 to 1.5 solar metallicity is consistent with modern determinations of the metallicity in the hot (T$\sim 10^{6}-10^{7}K$) ISM and the upper range of this warm ISM metallicity is consistent with stellar population metallicity determinations. A solar metallicity of the warm ISM favors an internal origin for the warm ISM such as AGB mass loss within the galaxy.Comment: Accepted Astrophysical Journa