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Biomedical subjects

H Campins

Publications and source records attributed to H Campins.

7 recordsLinked to original sources
PubMed2005

Deep Impact: observations from a worldwide Earth-based campaign.

On 4 July 2005, many observatories around the world and in space observed the collision of Deep Impact with comet 9P/Tempel 1 or its aftermath. This was an unprecedented coordinated observational campaign. These data show that (i) there was new material after impact that was compositionally different from that seen before impact; (ii) the ratio of dust mass to gas mass in the ejecta was much larger than before impact; (iii) the new activity did not last more than a few days, and by 9 July the comet's behavior was indistinguishable from its pre-impact behavior; and (iv) there were interesting transient phenomena that may be correlated with cratering physics.

Cosmic Dust↗
PubMed1993

Detection of the 2165 inverse centimeter (4.619 micron) XCN band in the spectrum of L1551 IRS 5.

We report the detection of a broad absorption band at 2165 cm-1 (4.619 microns) in the spectrum of L1551 IRS 5. New laboratory results over the 2200-2100 cm-1 wavenumber interval (4.55-4.76 microns), performed with realistic interstellar ice analogs, suggest that this feature is due to a CN-containing compound. We will refer to this compound as XCN. We also confirm the presence of frozen CO (both in nonpolar and polar matrices) through absorption bands at 2140 cm-1 (4.67 microns) and 2135 cm-1 (4.68 microns). The relative abundance of solid-state CO to frozen H2O is approximately 0.13 while the abundance of XCN seems comparable to that of frozen CO.

Astronomical Phenomena↗
PubMed1987

Airborne and groundbased spectrophotometry of comet P/Halley from 5-13 micrometers.

Spectrophotometry from 5-10 micrometers (delta lambda/lambda approximately 0.02) of comet Halley was obtained from the Kuiper Airborne Observatory on 1985 December 12.1 and 1986 April 8.6 and 10.5, UT. 8-13 micrometers data were obtained on 17.2 December 1985 from the Nickel Telescope at Lick Observatory. The spectra show a strong broad emission band at 10 micrometers and a weak feature at 6.8 micrometers. We do not confirm the strong 7.5 micrometers emission feature observed by the Vega 1 spacecraft. The 10 micrometers band, identified with silicate materials, has substructure indicative of crystalline material. The band can be fitted by combining spectra data from a sample of interplanetary dust particles. The primary component of the silicate emission is due to olivine. The 6.8 micrometers emission feature can be due either to carbonates or the C-H deformation mode in organic molecules. The lack of other emission bands is used to place limits on the types of organic molecules responsible for the emission observed by others at 3.4 micrometers. Color temperatures significantly higher than the equilibrium blackbody temperature indicate that small particles are abundant in the coma. Significant spatial and temporal variations in the spectrum have been observed and show trends similar to those observed by the spacecraft and from the ground. Temporal variability of the silicate emission relative to the 5-8 micrometers continuum suggests that there are at least two physically separated components of the dust.

Astronomical Phenomena↗
PubMed1980

Demonstration and quantification oomycosis.

Using a radioimmunoassay technique, we have determined the total IgE concentration and specific IgE antibody level against Paracoccidioides brasiliensis in the sera of patients with mycologically confirmed active paracoccidioidcosis. Patients with aspergilloma, or individuals with antibodies against Cadida albicans, and sera of apparently healthy individuals from the endemic area were also examined. The level of total IgE was significantly elevated in 9 out of 10 cases of paracoccidioidomycosis. The mean level of specific IgE against P. brasiliensis was significantly higher in the serum of the patients in comparison with control individuals. The percentage of specific IgE relative to the total varied from 0.38 to 2.28%. The differences between IgE levels in pare other mycoses were statistically significant. Our results suggest a possible involvement of specific IgE antibodies against P. brasiliensis in the immune response of patients with paracoccidioidomycosis. The hyperimmunoglobulinemia E may be related to the T-cell defect that characterizes the severe forms of the disease.

Adolescent↗
PubMed1975

[Cryptococcosis in Venezuela. Comments on a clinical case with unusual location].

A tumor like case of Cryptococcosis with a rare location in the abdomen of a young healthy woman is commented. It gave the opportunity to refer to the pathogeny of the disease, making in that way a brief review of the cases known in Venezuela and some not still published from which we got information. That review showed that generally doctors found more frequently organic lesions within the fields they are specially working for. It is obvious that mycosis must be considered in the diagnosis of nearly every patient in many countries and that laboratories must get appropriate equipment and personnel to help in that diagnosis.

Adolescent↗