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Planets found in and near the typically barren hot-Neptune `desert'1,2 (a region in mass-radius space that contains few planets) have proved to be particularly valuable in this regard. These planets include HD149026b3, which is thought to have an unusually massive core, and recent ...
A filamentary molecular gas structure, which is likely part of a larger molecular complex with VLSR~75-79 km/s, is detected and is found to surround the southern boundary of the remnant. In particular, the high-velocity wing (77-110 km/s) in the 12CO (J=1-0 and J=2-1) emission...
We aimed to: 1) define adipose tissue ontogeny of key proinflammatory and endoplasmic reticulum stress gene expression from late fetal to early adult life and 2) examine the impact on these genes in gestational nutrient restriction. Pregnant sheep were fed 100% (control) or 50% (NR) of their...
Park S. Nucleosynthesis in the oxygen-rich supernova remnant G292.0+1.8 from Chandra X-ray spectroscopy[J].Nuclear Instruments and Methods in Physics Research A:Accelerators,Spectrometers,Detectors and Associated Equipment,2004,(1.part2):144-148.doi:10.1086/382276.Park S., Hughes J. P., Slane...
The spectra and the size of the arc($\\mathrm{radius} \\approx 5\\degr$) are reasonably well explained by a model inwhich the arc is the bright edge of a $\\sim$100,000-yr old SNR located$\\sim$1--2 kpc above the disk. The agreement between the model and theobservations can ...
The Kostomuksha greenstone belt, NW Baltic Shield; remnant of a late Archaean oceanic plateau? Terra Nova 9 (2), 87-90.PUCHTEL I S,HOFMANN A W,JOCHUM K P,et al.The Kostomuksha greenstone belt, NW Baltic Shield: Remnant of a late Archaean oceanic plateau. Terra Nova . 1997...
We observed a nearby merger remnant NGC 7252 with the X-ray satellite ASCA and detected X-ray emission with the X-ray flux of (1.8 +- 0.3) x 10~(13) ergs s~(-1) cm~(-2) in the 0.5-10 keV band. This corresponds to the X-ray luminosity of 8.1 x 10~(40) ergs s~(-1)....
A NEW MECHANISM EXPLAINING THE ASYMMETRIC X-RAY EMISSION FROM SUPERNOVA REMNANT PKS 1209―52The interaction of a supernova remnant with its surrounding environment is a powerful source of radiation in various spectral regions and at different stages in its development. The study of these emissions ...