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  2. Temporary Error 14 in AOL Mail

    help.aol.com/articles/temporary-error-14-in-aol-mail

    Learn about possible workarounds for Temporary Error 14 in AOL Mail.

  3. 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 ...

  4. List of stellar properties - Wikipedia

    en.wikipedia.org/wiki/List_of_stellar_properties

    Download QR code; Print/export Download as PDF; Printable version; In other projects ... move to sidebar hide. Pages Related to Stellar properties, Pages using the ...

  5. Aberration (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Aberration_(astronomy)

    In astronomy, aberration (also referred to as astronomical aberration, stellar aberration, or velocity aberration) is a phenomenon where celestial objects exhibit an apparent motion about their true positions based on the velocity of the observer: It causes objects to appear to be displaced towards the observer's direction of motion.

  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. Stellar density - Wikipedia

    en.wikipedia.org/wiki/Stellar_density

    The true stellar density near the Sun is estimated as 0.004 stars per cubic light year, or 0.14 stars pc −3. When combined with estimates of the stellar masses, this yields a mass density estimate of 4 × 10 −24 g/cm 3 or 0.059 solar masses per cubic parsec. The density estimate varies across space, with the density decreasing rapidly in ...

  8. Stellar parallax - Wikipedia

    en.wikipedia.org/wiki/Stellar_parallax

    Stellar parallax is the basis for the parsec, which is the distance from the Sun to an astronomical object that has a parallax angle of one arcsecond. (1 AU and 1 parsec are not to scale, 1 parsec = ~206265 AU)

  9. Binary star - Wikipedia

    en.wikipedia.org/wiki/Binary_star

    The well-known binary star Sirius, seen here in a Hubble photograph from 2005, with Sirius A in the center, and white dwarf, Sirius B, to the left bottom from it. A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other.