Zobrazeno 1 - 10
of 17
pro vyhledávání: '"K D, Tucker"'
Publikováno v:
Journal of exposure analysis and environmental epidemiology. 7(1)
The Dietary Exposure Potential Model (DEPM) is a computer-based model developed for estimating dietary exposure to chemical residues in food. The DEPM is based on food consumption data from the 1987-1988 Nationwide Food Consumption Survey (NFCS) admi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::23eeec1718911fef29a8be45a22b88cb
https://pubmed.ncbi.nlm.nih.gov/9076611
https://pubmed.ncbi.nlm.nih.gov/9076611
Autor:
Tracy D. Wilkins, K D Tucker
Publikováno v:
Infection and immunity. 59(1)
Clostridium difficile causes pseudomembranous colitis in humans. The enterotoxin (i.e., toxin A) from this organism is believed to be responsible for the initial intestinal pathology associated with this disease. Previous work shows that this toxin b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa7467e175bb1cf91c6ccb4c77e47c20
https://pubmed.ncbi.nlm.nih.gov/1670930
https://pubmed.ncbi.nlm.nih.gov/1670930
Publikováno v:
IEEE Transactions on Nuclear Science. 21:776-783
A brief description of the EBR-II reactor and its supporting digital computer (which was designed to be transparent to the operator or experimenter) are discussed. Details of the system hardware and software are noted which allow the system to functi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83261be86f498f4fbb0133c6218b7c3a
https://doi.org/10.1109/tns.1974.4327549
https://doi.org/10.1109/tns.1974.4327549
Publikováno v:
The Journal of Chemical Physics. 59:131-135
The hfs of five rotational transitions of furan (C4H4O) has been resolved with a beam maser spectrometer with a resolution of about 500 Hz. All significant details of the observed structure are accounted for by the spin‐spin and spin‐rotation int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9bce1c60d0a914a4db50467987e5c35
https://doi.org/10.1063/1.1679780
https://doi.org/10.1063/1.1679780
Autor:
K. D. TUCKER, G. R. TOMASEVICH
Publikováno v:
Chemischer Informationsdienst. 5
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::409082821f5baf27868813c2d97490d7
https://doi.org/10.1002/chin.197416080
https://doi.org/10.1002/chin.197416080
Publikováno v:
Chemischer Informationsdienst. 4
The hfs of five rotational transitions of furan (C4H4O) has been resolved with a beam maser spectrometer with a resolution of about 500 Hz. All significant details of the observed structure are accounted for by the spin‐spin and spin‐rotation int
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::413fcf2ba12d7f41e3aff62d6a5e54e1
https://doi.org/10.1002/chin.197340088
https://doi.org/10.1002/chin.197340088
Publikováno v:
The Astrophysical Journal. 193:L115
Four new interstellar lines have been detected near 87.3 GHz. Based on laboratory ESR data these lines have been positively defined as hyperfine components of the lowest rotational transition of the ethynyl radical C2H. The observations gave precise
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fc8f9eed36e7a90a6f03142b1922304e
https://doi.org/10.1086/181646
https://doi.org/10.1086/181646
Publikováno v:
The Astrophysical Journal. 215:521
Line emission from CO at 2.6 mm is observed over an area of 28 square degrees in the Orion region. Most of the emission comes from two giant molecular complexes, roughly associated with Ori B and Ori A. The latter provides the best example of a giant
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9192df955a5e1e1fda84ee6590b92244
https://doi.org/10.1086/155384
https://doi.org/10.1086/155384
Publikováno v:
The Astrophysical Journal. 210:679
Emission from the J = 1-0 transition of carbon monoxide has been mapped over an area of 40 by 55 arcmin in cloud L134, and visual extinctions over the entire cloud have been obtained by means of star counts. Line intensities of at least 2 K are obser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19688808c1328ced84036cf03c14572a
https://doi.org/10.1086/154874
https://doi.org/10.1086/154874
Publikováno v:
The Astrophysical Journal. 209:452
H2CO emission at 2 mm is seen over a region 30 arcmin in extent which includes OMC-1 and OMC-2. The mass of this cloud, estimated from H2CO and CO observations, is about 7000 solar masses. The velocity pattern is one of rotation, with evidence for fr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::67e483dfccc2c3ed3295653905664df7
https://doi.org/10.1086/154739
https://doi.org/10.1086/154739