25 research outputs found
Gas-Rich Dwarf Galaxies from the PSS-II --- II. Optical Properties
We describe the optical properties of a sample of 101 gas-rich field dwarf
galaxies found on PSS-II (Second Palomar Sky Survey) plates, most newly
discovered as part of a survey to investigate the clustering properties of
dwarf galaxies relative to giants. These galaxies have low surface brightnesses
and are relatively distant, with recession velocities ranging up to 10,000
km/s. They have bluer V-I colors (median value of 0.75) than either actively
star-forming giant galaxies or low metallicity globular clusters, implying that
these dwarfs have both low metallicities and little past star formation. These
galaxies are also extremely gas rich, with a median HI mass to V luminosity
ratio of approximately 2 in solar units. We divide the sample into two groups:
true dwarfs with diameters (at 25 I mag arcsec^-2) less than 7.5 kpc and
Magellanic dwarfs with diameters greater than that value. The true dwarfs have
greater HI mass to V luminosity ratios and slightly bluer V-I colors than the
Magellanic dwarfs. Overall, the optical properties of our sample of dwarf
galaxies point towards their being quiescent objects that have undergone little
star formation over the age of the universe. They are not faded objects, but
instead may be going through one of their first periods of weak star formation.Comment: 27 pages, to appear in 20 May 1997 ApJ, paper also available at
http://www.astro.nwu.edu/astro/pildis/dwarfphot.html and
http://zebu.uoregon.edu/~js/dwarf.htm
Gas Rich Dwarfs from the PSS-II III. HI Profiles and Dynamical Masses
We present Arecibo neutral hydrogen data on a sample of optically selected
dwarf galaxies. The sample ranges in HI mass from 10^6 M_sun to 5x10^9 M_sun,
with a mean of 7.9x10^8 M_sun. Using estimated HI radii, the HI surface
densities range from 0.6 to 20 M_sun pc^-2, all well below the critical
threshold for star formation (Kennicutt 1998). M_HI/L values of the LSB dwarfs
range from 0.3 to 12 with a mean value of 2.0. Dynamical masses, calculated
from the HI profile widths, range from 10^8 M_sun to 10^11 M_sun. There is a
strong correlation between optical luminosity and dynamical mass for LSB dwarfs
implying that the dark matter (whether baryonic or non-baryonic) follows the
detectable baryonic matter.Comment: 53 pages, AASTeX v4.0, 8 figures, to be published in ApJ Suppl,
images, tables and referee report can be found at http://zebu.uoregon.edu/~j
Gas Mass Fractions and the Evolution of LSB Dwarf Galaxies
The optical and HI properties for a sample of low surface brightness (LSB)
dwarf galaxies, cataloged from the Second Palomar Sky Survey, is presented. Gas
mass fractions for LSB dwarfs reach the highest levels of any know galaxy type
(f_g=95%) confirming that their low stellar densities are due to inefficient
conversion of gas mass into stellar mass. Comparison with star formation models
indicates that the blue optical colors of LSB dwarfs is not due to low
metallicity or recent star formation and can only be explained by a dominant
stellar population that is less than 5 Gyrs in mean age. If star formation
occurs in OB complexes, similar to normal galaxies, then LSB dwarfs must
undergo weak bursts traveling over the extent of the galaxy to maintain their
LSB nature, which contributes to their irregular morphological appearance.Comment: 23 pages AAS LaTeX, 7 figures, accepted for publication in A
COVID-19 symptoms at hospital admission vary with age and sex: results from the ISARIC prospective multinational observational study
Background:
The ISARIC prospective multinational observational study is the largest cohort of hospitalized patients with COVID-19. We present relationships of age, sex, and nationality to presenting symptoms.
Methods:
International, prospective observational study of 60â109 hospitalized symptomatic patients with laboratory-confirmed COVID-19 recruited from 43 countries between 30 January and 3 August 2020. Logistic regression was performed to evaluate relationships of age and sex to published COVID-19 case definitions and the most commonly reported symptoms.
Results:
âTypicalâ symptoms of fever (69%), cough (68%) and shortness of breath (66%) were the most commonly reported. 92% of patients experienced at least one of these. Prevalence of typical symptoms was greatest in 30- to 60-year-olds (respectively 80, 79, 69%; at least one 95%). They were reported less frequently in children (â€â18 years: 69, 48, 23; 85%), older adults (â„â70 years: 61, 62, 65; 90%), and women (66, 66, 64; 90%; vs. men 71, 70, 67; 93%, each Pâ<â0.001). The most common atypical presentations under 60 years of age were nausea and vomiting and abdominal pain, and over 60 years was confusion. Regression models showed significant differences in symptoms with sex, age and country.
Interpretation:
This international collaboration has allowed us to report reliable symptom data from the largest cohort of patients admitted to hospital with COVID-19. Adults over 60 and children admitted to hospital with COVID-19 are less likely to present with typical symptoms. Nausea and vomiting are common atypical presentations under 30 years. Confusion is a frequent atypical presentation of COVID-19 in adults over 60 years. Women are less likely to experience typical symptoms than men