Biomedical subjects

C Baumstark-Khan

Publications and source records attributed to C Baumstark-Khan.

23 records · Page 2Linked to original sources

PubMed1986

Radiation induced formation of giant cells in Saccharomyces uvarum. IV. Macromolecular synthesis and protein patterns.

X-irradiated (1.0 kGy) yeast cells (Saccharomyces uvarum, ATCC 9080), grown in liquid medium stop their mitotic activities and form giant cells by development of several buds which do not separate from mother cells. Depending on the time in culture, wet and dry weights per cell, protein-RNA- and DNA- contents per cell as well as incorporation rates of 14C-leucine per cell and per hour and patterns (isoelectric focussing) of water soluble proteins were studied. Weights per cell, RNA and protein contents per cell and 14C-leucine incorporation rates increase markedly in giant cells, whereas DNA content per cell is only duplicated. Protein patterns in isoelectric focusing show one interesting difference. In samples from giant cells one protein band (IP = 6.63) decreases after 8 h in culture and later on disappears completely. This finding is not due to primary damage in X-irradiated DNA but seems to be related to the control of cell cycle events.

DNA, Fungal↗

PubMed1985

Radiation induced formation of giant cells in Saccharomyces uvarum. II. Effect of X-rays on septum formation.

Thin sections of budding yeast cells and giant gells grown after X-irradiation have been examined by electron microscopy. The different steps of cross-wall formation during budding were documented with unirradiated cells. With X-ray induced giant cells cytokinesis was shown to be absent. Neither primary nor secondary septae appeared thus cell separation did not occur. Despite this fact both macromolecular synthesis and bud growth continued, giving rise to the formation of giant cells.

Cell Wall↗

PubMed1984

Radiation induced formation of giant cells (Saccharomyces uvarum). I. Budding process and chitin ring formation.

X-irradiated yeast cells (Saccharomyces uvarum) grown in liquid media stop mitosis and form giant cells. Chitin ring formation, being a prerequisite for cell separation, was studied by fluorescence microscopy using calcofluor white, a chitin specific dye. Experiments with inhibitors of DNA synthesis (hydroxyurea) and chitin synthesis (polyoxin D) demonstrate chitin ring formation to be dependent on DNA synthesis, whereas bud formation is independent of DNA synthesis and chitin ring formation respectively. Basing on these results the formation of X-ray induced giant cells implies one DNA replication which in turn induces the formation of only one chitin ring between mother cell and giant bud. Obviously no septum can be formed. Thus cell separation does not occur, but the bud already formed, produces another bud demonstrating that bud formation itself is independent of DNA synthesis.

Cells, Cultured↗

PubMed1984

Monitoring yeast spindles in the fluorescence microscope.

Formation of the complete spindles during the budding process of Saccharomyces uvarum was investigated by fluorescence microscopy of protoplasted cells. Protoplasts were treated with anti-tubulin antibodies and DAPI, a fluorescent dye staining DNA. Thus, both chromatin and spindles could be visualized. Duplication as well as formation of separated spindle pole bodies during the different stages of budding are documented, demonstrating the occurrence and behaviour of microtubules during yeast cell cycle.

Antibodies↗

PubMedDate not supplied

Critical issues in connection with human planetary missions: protection of and from the environment.

Activities associated with human missions to the Moon or to Mars will interact with the environment in two reciprocal ways: (i) the mission needs to be protected from the natural environmental elements that can be harmful to human health, the equipment or to their operations: (ii) the specific natural environment of the Moon or Mars should be protected so that it retains its value for scientific and other purposes. The following environmental elements need to be considered in order to protect humans and the equipment on the planetary surface: (i) cosmic ionizing radiation, (ii) solar particle events; (iii) solar ultraviolet radiation; (iv) reduced gravity; (v) thin atmosphere; (vi) extremes in temperatures and their fluctuations; (vii) surface dust; (viii) impacts by meteorites and micrometeorites. In order to protect the planetary environment. the requirements for planetary protection as adopted by COSPAR for lander missions need to be revised in view of human presence on the planet. Landers carrying equipment for exobiological investigations require special consideration to reduce contamination by terrestrial microorganisms and organic matter to the Greatest feasible extent. Records of human activities on the planet's surface should be maintained in sufficient detail that future scientific experimenters can determine whether environmental modifications have resulted from explorations. Grant numbers: 14056/99/NL/PA.

Aerospace Medicine↗