نتایج جستجو برای: m15

تعداد نتایج: 598  

2000
L. Sidoli A. N. Parmar T. Oosterbroek

Results of a 1999 November 16–17 BeppoSAX observation of the low-mass X-ray binary X 2127+119 located in the globular cluster M15 are presented. The system is believed to be one where the central neutron star is normally obscured by the accretion disk, and only X-rays scattered into our line of sight by an extended accretion disk corona (ADC) are observed. The 0.1–10 keV lightcurve is energy de...

2017
Suh-Ching Yang Shyh-Hsiang Lin Jung-Su Chang Yi-Wen Chien

The aim of this study was to investigate the effect of a high fat diet with experimental oil consisting of 60% MUFAs (monounsaturated fatty acids) with a P/S ratio of 5 on fat deposition and lipid metabolism in obese hamsters. Hamsters were randomly assigned to a control group and a diet-induced obesity group for nine weeks. Then an additional eight-week experimental period began, during which ...

2006
José Luis Prieto Nicholas B. Suntzeff

We present a new empirical method for fitting multicolor light curves of Type Ia supernovae. Our method combines elements from two widely used techniques in the literature: the ∆m15 template fitting method (Phillips et al. 1999) and the Multicolor Light-Curve Shape method (MLCS; Riess, Press, & Kirshner 1996). An advantage of our technique is the ease of adding new colors, templates, or paramet...

2009
WILLIAM A. BAUM ROGER LYNDS

We have obtained U-band images of the M15 core with the Planetary Camera of the Hubble Space Telescope. We are able to resolve stars down to the main-sequence turnoff (mu ~ 19.4) into the cluster center. We use crowded field photometry techniques to decompose M15 into bright resolved stars and a residual component consisting of stars at turnoff brightness or fainter. The residual component comp...

2000
L. Sidoli A. N. Parmar

Results of a 1999 November 16–17 BeppoSAX observation of the low-mass X-ray binary X 2127+119 located in the globular cluster M15 are presented. The system is believed to be one where the central neutron star is normally obscured by the accretion disk, and only X-rays scattered into our line of sight by an extended accretion disk corona (ADC) are observed. The 0.1–10 keV lightcurve is energy de...

Journal: :Bulletin of the World Health Organization 1995
F O ter Kuile F Nosten C Luxemburger D Kyle P Teja-Isavatharm L Phaipun R Price T Chongsuphajaisiddhi N J White

Between 1990 and 1994, a series of prospective studies were conducted to optimize the treatment of multidrug-resistant falciparum malaria on the borders of Thailand. The tolerance of various treatment regimens containing either mefloquine 15 mg/kg (M15) or 25 mg/kg (M25) was evaluated in 3673 patients aged between 6 months and 88 years. Early vomiting (within 1 hour) is an important determinant...

2004
L. van Zyl P. A. Charles S. Arribas T. Naylor E. Mediavilla C. Hellier

We present integral field spectroscopy of X2127+119, the luminous X-ray binary in the globular cluster M15, obtained with INTEGRAL/WYFFOS on the William Herschel Telescope. We find that tomograms of He II λ4686 line profiles appear to be incompatible with the previously-assumed view of X2127+119, in which the binary consists of a 1.4-M⊙ neutron star and a 0.8-M⊙ sub-giant companion near the mai...

Journal: :The Biochemical journal 1995
M L Bonet F Serra J C Matamala F J García-Palmer A Palou

The relative stability against a decrease in adrenergic stimulation of the uncoupling protein (UCP) incorporated into different mitochondrial fractions was investigated in brown-fat-cell cultures. Cultures were initiated with undifferentiated cells from young mice and were acutely stimulated with noradrenaline at confluence (day 7). Cells were harvested just after the finish of the 24 h stimula...

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