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...not easily push high density clouds. As the cosmic winds start to push the clouds, they start to separate and start looking like taffy being pulled apart.<re ...w [[Redshift|redshifts]] of ultraviolet star forming galaxies, the outflow velocity and mass loading factor of the wind, scale with the star formation rate (SF ...

...cities which are measured in excess of 70–90&nbsp;km s⁻¹. These clouds of gas can be massive in size, some on the order of millions of times the [ ...amount of [[baryonic matter]] in the galactic halo. In addition, as these clouds fall into the disk of the galaxy, they add material that can form stars in ...

| discovery_method = [[Doppler spectroscopy|Radial velocity]] ...Neptune]] from the Sun) with a period of around 180 years and a relatively high [[orbital eccentricity|eccentricity]] of 0.4, and has a mass around seven t ...

...ion, but this is not true in star forming regions where the gas density is high and the degree of ionization is low.{{Citation needed|reason=Because of the ...can produce dense regions, but they cannot by themselves make the density high enough for self-gravity to act. However, the [[gas]] in star forming region ...

...ds.<ref name="supernova" /> A 2014 study measured that Henize 70 featured high S_II and Hα ratios, indicating that it is not a supernova remnant ...13 February 2012|title=The Optical Depth of H II Regions in the Magellanic Clouds|journal=The Astrophysical Journal|volume=755|issue=1|pages=30|bibcode=2012A ...

...that possess deep convective cores enmeshed in low altitude precipitative clouds.<ref>{{cite journal |author = Houze, R. a, Chen, S. S., Smull, B. F., Lee, ...s a good indicator of overall intensity due to an increase in [[rotational velocity]] when the distance between the moving particles and the center of the vort ...

...isturbances will relate to the initial properties of the system, such as [[velocity]], [[pressure]], and [[density]]. [[James Clerk Maxwell]] expressed the qua | <math>u</math> is the velocity of the fluid flow ...

...ity of 3,100&nbsp;km/sec at the distance of the SMC, well above its escape velocity. A more likely explanation of such a proper motion would be that HV 2112 li ...2 in the Small Magellanic Cloud. The star was thought to contain unusually high levels of the elements [[lithium]], [[molybdenum]] and [[rubidium]] that ar ...

| radial_v = <!--Radial velocity (in km/s)--> ...ered by [[Kevin Luhman]] in March 2013, who noticed the object's unusually high [[proper motion]] while searching for [[Nemesis (hypothetical star)#Past, c ...

...by using the integrated [[radio waves|radio emission]] from unresolved gas clouds. ...977SvAL....3..155V}}</ref> calculate the effect of 21cm line absorption at high redshift on the spectrum of the CMB. ...

...6-AIAA-2016-0999.pdf |title=Airborne Observations of an Asteroid Entry for High Fidelity Modeling: Space Debris Object WT1190F |last=Jenniskens |first=Petr ...y]] utilized a [[Gulfstream 450]] jet to study the re-entry from above the clouds and haze.<ref name=UAE/> The airborne observation team successfully capture ...

...hnologies, as it allows the manipulation of light-matter interactions with high precision. Detuning has use cases in research fields including [[quantum op ...>\vec{k}</math> is the laser's wave vector and <math>\vec{v}</math> is the velocity of the atom. Engineering the laser detuning in this way to a specific red s ...

...uld seed other planetary systems, [[protoplanetary disc]]s or star-forming clouds with [[microorganism]]s, to secure and expand its organic gene/protein life ...Directed panspermia. 3. Strategies and motivation for seeding star-forming clouds | journal = J. British Interplanetary Soc. | volume = 50 | pages = 93–102 | ...

...channel is not uniform. The fluid travels in a parabolic pattern with the velocity of the flow, increasing with the distance from the walls up towards the cen ...J. Calvin Giddings]]. The technique is based on separation of colloidal or high molecular weight substances in liquid solutions, flowing through the separa ...

...uments have been used to study, among other, atmospheric gases, aerosols, clouds, and temperature. | title = Apparatus for determining light characteristics of clouds by reflection ...

...-3-540-68322-3_2|isbn=978-3-540-24430-1|access-date=2021-06-24}}</ref> The high variability of the ocean surface is also the deterministic factor in the di ...continuation. The [[Advanced very-high-resolution radiometer|Advanced Very-High-Resolution Radiometer]] (AVHRR) Is the sensor carried on al [[National Ocea ...

...st8=E.|title=Properties of luminous red supergiant stars in the Magellanic Clouds|journal=[[Astronomy and Astrophysics]]|year=2023 |volume=669 |pages=17|doi= ...er>{{cite journal|bibcode=2004ApJ...605..436M|arxiv=astro-ph/0401363|title=High-Resolution Imaging of Dust Shells by Using Keck Aperture Masking and the IO ...

...ubble. Other SBSL theories explain that the emission of photons due to the high temperatures in the bubble are analogical to the hot spot theories of MBSL. ...ence. The bright blue dots, which are viewable when the image is viewed at high resolution are the sonoluminescencing bubbles.]] ...

...te=July 1995 |title=Ions in the terrestrial atmosphere and in interstellar clouds |url=https://analyticalsciencejournals.onlinelibrary.wiley.com/doi/10.1002/ ...not fully understood. However, it can be elucidated that it may form under high methane density conditions and, probably, a [[Three-body problem|three body ...

...tinguish|Space velocity (astronomy)|radial velocity|proper motion|peculiar velocity}} Stellar kinematics encompasses the measurement of stellar [[Velocity|velocities]] in the [[Milky Way]] and its [[Satellite galaxies of the Milky ...