enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Interstellar medium - Wikipedia

    en.wikipedia.org/wiki/Interstellar_medium

    There is some 'dark gas', regions where hydrogen is in molecular form and therefore does not emit the 21-cm line, but CO molecules are broken up so the CO lines are also not present. These regions are inferred from the presence of dust grains with no matching line emission from gas. [14]

  3. List of interstellar and circumstellar molecules - Wikipedia

    en.wikipedia.org/wiki/List_of_interstellar_and...

    The molecules listed below were detected through astronomical spectroscopy. Their spectral features arise because molecules either absorb or emit a photon of light when they transition between two molecular energy levels. The energy (and thus the wavelength) of the photon matches the energy difference between the levels involved.

  4. Interstellar cloud - Wikipedia

    en.wikipedia.org/wiki/Interstellar_cloud

    A map of the abundance of these molecules can be made, enabling an understanding of the varying composition of the clouds. In hot clouds, there are often ions of many elements , whose spectra can be seen in visible and ultraviolet light .

  5. Molecular cloud - Wikipedia

    en.wikipedia.org/wiki/Molecular_cloud

    The discovery of the 21 cm line was the first step towards the technology that would allow astronomers to detect compounds and molecules in interstellar space. [3] Plaque commemorating the discovery of 21-cm radiation from the Milky Way. In 1951, two research groups nearly simultaneously discovered radio emission from interstellar neutral hydrogen.

  6. Water hole (radio) - Wikipedia

    en.wikipedia.org/wiki/Water_hole_(radio)

    The waterhole, or water hole, is an especially quiet band of the electromagnetic spectrum between 1420 and 1662 megahertz, corresponding to wavelengths of 18–21 centimeters. It is a popular observing frequency used by radio telescopes in radio astronomy .

  7. H I region - Wikipedia

    en.wikipedia.org/wiki/H_I_region

    (H is the chemical symbol for hydrogen, and "I" is the Roman numeral. It is customary in astronomy to use the Roman numeral I for neutral atoms, II for singly-ionized—HII is H + in other sciences—III for doubly-ionized, e.g. OIII is O ++ , etc. [ 1 ] ) These regions do not emit detectable visible light (except in spectral lines from ...

  8. Ionized-air glow - Wikipedia

    en.wikipedia.org/wiki/Ionized-air_glow

    When energy is deposited in air, the air molecules become excited. As air is composed primarily of nitrogen and oxygen, excited N 2 and O 2 molecules are produced. These can react with other molecules, forming mainly ozone and nitrogen(II) oxide. Water vapor, when present, may also play a role; its presence is characterized by the hydrogen ...

  9. Hydrogen line - Wikipedia

    en.wikipedia.org/wiki/Hydrogen_line

    A hydrogen atom with proton and electron spins aligned (top) undergoes a flip of the electron spin, resulting in emission of a photon with a 21 cm wavelength (bottom) The hydrogen line, 21 centimeter line, or H I line [a] is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms.