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  2. Molecular cloud - Wikipedia

    en.wikipedia.org/wiki/Molecular_cloud

    A molecular cloud, sometimes called a stellar nursery (if star formation is occurring within), is a type of interstellar cloud, the density and size of which permit absorption nebulae, the formation of molecules (most commonly molecular hydrogen, H 2), and the formation of H II regions.

  3. Serpens–Aquila Rift - Wikipedia

    en.wikipedia.org/wiki/Serpens–Aquila_Rift

    The molecular cloud at these wavelengths is traced by emission from warm dust in the clouds, allowing the structure of the clouds to be probed. Wavelet analysis of the molecular clouds in the approximately 11 square degree Herschel field of view breaks up the clouds into numerous filaments, mostly in and around the Westerhout 40 region. [20]

  4. Vela Molecular Ridge - Wikipedia

    en.wikipedia.org/wiki/Vela_Molecular_Ridge

    The B cloud of the Vela Molecular Ridge is a structure independent of the others, located at about 2000 parsecs in a remote and peripheral region of the Orion Arm. In it are contained 7 of the infrared sources associated with objects of Class I, none of which has been studied in detail. [ 2 ]

  5. Did a 'giant molecular cloud' kill off the dinosaurs?

    www.aol.com/news/2016-03-29-did-a-giant...

    A new study proposes that the dinosaurs were killed off due to severe global cooling caused when the Earth passed through a ‘giant molecular cloud.’

  6. Westerhout 40 - Wikipedia

    en.wikipedia.org/wiki/Westerhout_40

    These filaments of cloud have dense "cores" of gas embedded within them—many of which are likely to gravitationally collapse and form stars. The Herschel results for this region, and subsequently reported results for other star-forming regions, imply that fragmentation of molecular-cloud filaments are fundamental to the star-formation process.

  7. Chamaeleon complex - Wikipedia

    en.wikipedia.org/wiki/Chamaeleon_complex

    The cloud is sometimes extended with an eastern part, [18] and together with the distinctively long Dark Doodad Nebula (or Musca nebula) to the north the complex is called the Musca-Chamaeleonis Molecular Cloud. [19] Two foreground associations are found near the Chamaeleon dark clouds.

  8. Maggie (astronomy) - Wikipedia

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

    Maggie is a vast cloud of hydrogen gas observed within our own Milky Way galaxy. It is a filament of hydrogen 3,900 light-years long and 130 light-years wide. It is a single coherent structure with all parts showing similar velocity with respect to the local standard of rest. It is one of the biggest structures within the Milky Way.

  9. Update on Little Blind Dachshund Who Needs a Home for the ...

    www.aol.com/little-blind-dachshund-needs-home...

    It was the woman's mission to find the Dachshund a home before the holidays. And what better way to do so than by sharing a video of the dog in his kennel and giving him an introduction to the ...