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  2. DLL hell - Wikipedia

    en.wikipedia.org/wiki/DLL_Hell

    DLL hell is an umbrella term for the complications that arise when one works with dynamic-link libraries (DLLs) used with older Microsoft Windows operating systems, [1] particularly legacy 16-bit editions, which all run in a single memory space. DLL hell can appear in many different ways, wherein affected programs may fail to run correctly, if ...

  3. Dynamic-link library - Wikipedia

    en.wikipedia.org/wiki/Dynamic-link_library

    A dynamic-link library (DLL) is a shared library in the Microsoft Windows or OS/2 operating system. A DLL can contain executable code (functions), data, and resources. A DLL file often has file extension.dll even though this is not required. The extension is sometimes used to describe the content of the file.

  4. KIK-30 - Wikipedia

    en.wikipedia.org/wiki/KIK-30

    The KIK-30 "Really Simple Key loader" (RASKL) is a fill device made by Sypris Electronics and approved by the US National Security Agency for the distribution of NSA Type 1 cryptographic keys. It can also store and transfer related communications security material, including control data ("load sets") for frequency hopping radios, such as ...

  5. HD 140283 - Wikipedia

    en.wikipedia.org/wiki/HD_140283

    [1] [13] However, more recent models of its stellar evolution have suggested revision of the star's age to 13.7 billion years [14] or 12 billion years. [ 5 ] Dubbed the " Methuselah Star" by the popular press due to its age, [ 15 ] [ 16 ] the star must have formed soon after the Big Bang [ 1 ] and is one of the oldest stars known as of 2021. [ 5 ]

  6. Stellar wind - Wikipedia

    en.wikipedia.org/wiki/Stellar_wind

    A stellar wind is a flow of gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars by being less collimated , although stellar winds are not generally spherically symmetric.

  7. 14 Andromedae b - Wikipedia

    en.wikipedia.org/wiki/14_Andromedae_b

    14 Andromedae b (abbreviated 14 And b), formally named Spe / ˈ s p iː /, is an exoplanet approximately 249 light years away in the constellation of Andromeda. The 186-day period planet orbits about 83% the Earth-Sun distance from the giant star 14 Andromedae. It has a minimum mass 4.8 times the mass of Jupiter.

  8. Color index - Wikipedia

    en.wikipedia.org/wiki/Color_index

    In astronomy, the color index is a simple numerical expression that determines the color of an object, which in the case of a star gives its temperature.The lower the color index, the more blue (or hotter) the object is.

  9. Messier 62 - Wikipedia

    en.wikipedia.org/wiki/Messier_62

    The density profile of its member stars suggests it has not yet undergone core collapse. [14] It has a core radius of 1.3 ly (0.39 pc), a half-mass radius of 9.6 ly (2.95 pc), and a half-light radius of 6.0 ly (1.83 pc). The stellar density at the core is 5.13 M ☉ per cubic parsec. [15] It has a tidal radius of 59 ly (18.0 pc). [8]