2000
DOI: 10.1007/978-3-642-58813-6_11
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Tumour pH

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Cited by 9 publications
(6 citation statements)
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“…If the fraction of binary MACHOs is as high as that of binary stars, 5 ∼ 10 % of events are expected to be a caustic crossing event (Mao & Paczynski 1991). Thus, one can expect a caustic crossing event per a few year even with the current microlensing search, and if the next generation microlensing search is launched, the expected number of such an event will be increased by two order of magnitudes (Stubbs 1998). Therefore in a decade or so, we may be able to measure the MACHO mass for a number of events by combining the ground-based monitoring and the HST or other space telescope in the next generation.…”
Section: Discussionmentioning
confidence: 99%
“…If the fraction of binary MACHOs is as high as that of binary stars, 5 ∼ 10 % of events are expected to be a caustic crossing event (Mao & Paczynski 1991). Thus, one can expect a caustic crossing event per a few year even with the current microlensing search, and if the next generation microlensing search is launched, the expected number of such an event will be increased by two order of magnitudes (Stubbs 1998). Therefore in a decade or so, we may be able to measure the MACHO mass for a number of events by combining the ground-based monitoring and the HST or other space telescope in the next generation.…”
Section: Discussionmentioning
confidence: 99%
“…However, as for the TBF effects induced by hyperthermia, further investigations are required to define the real effects (short-or long-lasting oxygenation) as well as the underlying mechanisms [139]. Concerning tumor pH, one has to differentiate the extracellular pH (pH e ) from the intracellular one (pH i ) [136,149]. The effects of heating seemed to favor a decrease of both pH i and pH e , which in turn leads to an improvement of hyperthermia by sensitizing tumor cells [139].…”
Section: Tumor Metabolic Microenvironmentmentioning
confidence: 99%
“…Of the eight microlensing events detected by Alcock et al (1997b) during their first two years of observations, none of the sources were brighter than V = 20 (after removing blended light) which is the nominal limit for SIM. Future microlensing surveys could improve the rate of detection by an order of magnitude (Gould 1999b;Stubbs 1998). However, only a factor of three of this improvement would be due to the coverage of a larger area.…”
Section: Lmcmentioning
confidence: 99%