Namanya Kugy. Mungil, pengkhayal, dan berantakan. Dari benaknya, mengalir untaian dongeng indah. Keenan belum pernah bertemu manusia seaneh itu .... Namanya Keenan. Cerdas, artistik, dan penuh kejutan. Dari tangannya, mewujud lukisan-lukisan magis. Kugy belum pernah bertemu manusia seajaib itu .... Dan kini mereka berhadapan di antara hamparan misteri dan rintangan. Akankah dongeng dan lukisan itu bersatu? Akankah hati dan impian mereka bertemu?
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Tersedia di Perpustakaan Universitas Pelita Bangsa
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KASIH... Dari semua buku yang sudah saya terbitkan, harus saya akui bahwa
Perahu Kertas memiliki kedekatan ekstra dibandingkan yang lainnya. Ia bersama
saya sejak 1996, sejak saya masih duduk di bangku kuliah. Kisah ini pun sudah
...
The Space Plasma Wave Group within the Department of Physics and Astronomy at the University of Iowa in Iowa City, Iowa, provides information about the Very-Late-Type Spiral and Irregular Galaxy Supernova Search project. The purpose of the project is to discover new supernovae in very-late-type and irregular galaxies. The rates of occurrence of supernovae of different types is to be determined. Images of supernovae are available.
The purpose of the project is to discover new supernovae in very-late-type and irregular galaxies. The rates of occurrence of supernovae of different types is to be determined. Images of supernovae are available.
Gamma-ray line emission is a direct probe of the nucleosynthesis that occurs in Type Ia supernovae. In this work we describe the wealth of information obtainable from observations of this emission. Advanced Compton telescope designs are being studied by the Naval Research Laboratory, with the goal being the construction of a telescope which would be capable of detecting SNe Ia to distances in excess of 100 Mpc. We describe the instrument capabilities and the design issues that are being addressed. We assume a SN Ia rate and quantify the frequency at which an advanced Compton telescope could detect, discriminate between, and diagnose Type Ia supernovae. From these estimates, we argue that an advanced Compton telescope would be a powerful astrophysical tool.
Gamma-ray line emission is a direct probe of the nucleosynthesis that occurs in Type Ia supernovae. In this work we describe the wealth of information obtainable from observations of this emission.
