Starburst Mid-Flight: As the Dust Clears
نویسندگان
چکیده
The Starburst project, at IBM’s Almaden Research Center, is improving the design of relational database management systems and enhancing their performance, while building an extensible system to better support nontraditional applications (such as engineering, geographic, office, etc.), and to serve as a testbed for future improvements in database technology. As of November 1989, we have an initial prototype of our system up and running. In this paper, we reflect on the design and implementation of the Starburst system to date. We examine some key design decisions, and how they affect the goal of improved structure and performance. We also examine how well we have met our goal of extensibility: what aspects of the system are extensible, how extensions can be done, and how easy it is to add extensions. We discuss some actual extensions to the system, including the experiences of our first real customizers.
منابع مشابه
Mid - infrared and optical spectroscopy of ultraluminous infrared galaxies : A comparison
New tools from Infrared Space Observatory (ISO) mid-infrared spectroscopy have recently become available to determine the power sources of dust-obscured ultraluminous infrared galaxies (ULIRGs). We compare ISO classifications – starburst or active galactic nucleus (AGN) – with classifications from optical spectroscopy, and with optical/near-infrared searches for hidden broad-line regions. The a...
متن کاملMassive Star Formation in Galaxies : Radiative transfer models of the UV to mm emission of starburst galaxies .
We present illustrative models for the UV to millimeter emission of starburst galaxies which are treated as an ensemble of optically thick giant molecular clouds (GMCs) centrally illuminated by recently formed stars. The models follow the evolution of the GMCs due to the ionization-induced expansion of the HII regions and the evolution of the stellar population within the GMC according to the B...
متن کاملDust-to-gas ratios in the starburst regions of luminous infrared galaxies
We investigate the properties of dust and dust-to-gas ratios in different starburst regions of luminous infrared galaxies (LIGs). We refer to the sample of seven LIGs recently observed in the mid-infrared by Soifer et al. (2001) using the Keck telescopes with spatial resolution approaching the diffraction limit. These seven objects are among the closest LIGs and have been classified as starburs...
متن کاملStarburst and cirrus models for submillimeter galaxies
We present radiative transfer models for submillimeter galaxies with spectroscopic redshifts and mid-infrared spectroscopy from Spitzer/IRS and analyze available Spitzer/MIPS 24, 70 and 160μm data. We use two types of starburst models, a cirrus model and a model for the emission of an AGN torus in order to investigate the nature of these objects. We find that for three of the objects (25%) cirr...
متن کاملMid-infrared and Optical Spectroscopy of Ultraluminous Infrared Galaxies: a Comparison 1
New tools from Infrared Space Observatory (ISO) mid-infrared spectroscopy have recently become available to determine the power sources of dust-obscured ultraluminous infrared galaxies (ULIRGs). We compare ISO classiications { starburst or active galactic nucleus (AGN) { with classiications from optical spectroscopy, and with optical/near-infrared searches for hidden broad-line regions. The agr...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
- IEEE Trans. Knowl. Data Eng.
دوره 2 شماره
صفحات -
تاریخ انتشار 1990