2,659 research outputs found
Development of a Web-based software tool for predicting the occurrence and effect of air pollutants inside museum buildings
22-27 September 200
Air pollutant levels in air-conditioned and naturally ventilated museums: a pilot study
An air-conditioned and a naturally ventilated museum in a highly polluted part of London were compared for effectiveness of pollution control. Nitrogen dioxide, sulphur dioxide and hydrogen sulphide concentrations were measured inside and outside using diffusion tubes. Airborne particles were measured using a Grimm laser counting device. It was found that the benefits normally attributed to air-conditioning with filtration were not as great as might be thought. Only nitrogen dioxide and particle levels were significantly lower in the air-conditioned museum than in the naturally ventilated museum
Interstellar Mg II and C IV absorption by 1 1/2 galaxies along the sightline to MrK 205
The first results of our HST survey designed to search for Mg 2 and C 4 absorption lines from the disks and halos of low-redshift galaxies using background QSO's and supernovae as probes are presented. Our survey utilizes the high resolution of the Goddard High Resolution Spectrograph enabling us to calculate the column densities and doppler parameters of individual components within an absorption complex, and hence determine the physical conditions of the absorbing gas. Observing the complexity of the absorption line profiles i.e., the velocity distribution and total velocity extent of the constituent components, offers an important description of the kinematics of the absorbing gas, and hence an understanding of its origin. Focus is on one sight line in particular, that towards Mrk 205, which passes 3-5 kpc from the intervening galaxy NGC 4319. Mg 2 and C 4 absorption from both local Milky Way halo gas and from NGC 4319 is detected
The Detection of Lyman-alpha Absorption from Nine Nearby Galaxies
We have used STIS aboard HST to search for Lyman-alpha (Lya) absorption in
the outer regions of nine nearby (cz<6000 km/s) galaxies using background QSOs
and AGN as probes. The foreground galaxies are intercepted between 26 and 199
h-1 kpc from their centers, and in all cases we detect Lya within +/-500 km/s
of the galaxies' systemic velocities. The intervening galaxies have a wide
range of luminosities, from M_B = -17.1 to -20.0, and reside in various
environments: half the galaxies are relatively isolated, the remainder form
parts of groups or clusters of varying richness. The equivalent widths of the
Lya lines range from 0.08 - 0.68 A and, with the notable exception of
absorption from one pair, crudely correlate with sightline separation in a way
consistent with previously published data, though the column densities derived
from the lines do not. The lack of correlation between line strength and galaxy
luminosity or, in particular, the environment of the galaxy, suggests that the
absorption is not related to any individual galaxy, but arises in gas which
follows the same dark-matter structures that the galaxies inhabit.Comment: 8 pages, invited review to appear in the proceedings of the Yale
Cosmology Workshop on `The Shapes of Galaxies & their Halos", P. Natarajan,
ed. Best figures found in (17Mb) PS file at
http://astro.princeton.edu/~dvb/yale.p
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