Results 121 to 130 of about 5,067 (228)

Interstellar Cloud Material: Contribution to Planetary Atmospheres

, 1978
A statistical analysis of the properties of dense interstellar clouds indicates that the solar system has encountered at least a dozen clouds of sufficient density to cause planets to accumulate nonnegligible amounts of some isotopes.
Newman, Michael J., Butler, Dixon M., Talbot, Raymond J., Jr.   +2 more
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Profiles of interstellar cloud filaments

, 2012
Context. Sub-millimetre observations suggest that the filaments of interstellar clouds have rather uniform widths and can be described with the so-called Plummer profiles.
T. Lunttila, M. Juvela, J. Malinen
core   +1 more source

Discovery of Thionylimide, HNSO, in Space: The first N-, S-, and O-bearing Interstellar Molecule

The Astrophysical Journal Letters
We present the first detection in space of thionylimide (HNSO) toward the Galactic center molecular cloud G + 0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular line survey carried out with the Yebes 40 m and IRAM 30 m telescopes ...
Miguel Sanz-Novo, Víctor M. Rivilla, Holger S. P. Müller, Izaskun Jiménez-Serra, Jesús Martín-Pintado, Laura Colzi, Shaoshan Zeng, Andrés Megías, Álvaro López-Gallifa, Antonio Martínez-Henares, Belén Tercero, Pablo de Vicente, David San Andrés, Sergio Martín, Miguel A. Requena-Torres   +14 more
doaj   +1 more source

Dynamics of the Oort cloud and formation of interstellar comets

, 2020
The solar system was formed approximately 4.56 billion years ago. Despite the numerous theories that have been developed over the years, the formation and evolution of the solar system still remain unclear.To better understand the formation and evolution
Torres Rodriguez, S.
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Multi-wavelength View of the Interstellar Medium in the Large Magellanic Cloud

, 1998
The Large Magellanic Cloud (LMC) has been surveyed in optical emission lines, X-rays, radio continuum, HI, and CO lines. These surveys provide views of the interstellar medium (ISM) in the LMC of unprecedented clarity, allowing us to study astrophysical ...
You-Hua Chu
core   +1 more source

Novel algorithms for the understanding of the chemical cosmos

, 2015
Molecular data from the interstellar medium (ISM) contain information that holds the key to understanding our chemically controlled cosmos and to unlocking the secrets of our universe.
Makrymallis, A
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Heliospheric Response to Different Possible Interstellar Environments

, 2006
At present, the heliosphere is embedded in a warm, low-density interstellar cloud that belongs to a cloud system flowing through the local standard of rest with a velocity near ~18 km s-1. The velocity structure of the nearest interstellar material (ISM),
Hans‐Reinhard Muller, Florinski, Vladimir, Priscilla C. Frisch, Gary P. Zank, Muller, Hans-Reinhard, Zank, Gary P, Vladimir Florinski, Frisch, Priscilla C   +7 more
core   +1 more source

The interstellar polarization law [PDF]

, 1981
The work discussed in this thesis aimed to investigate the interstellar polarization law [p(lambda)/p[max] = exp (-K 2n[2]([lambda]max/(lambda)] and the behaviour of its characteristic parameters, K and lambda[max], in both max simple and complex cloud ...
Al-Roubaie, Alia Hussain Ali
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Unusual relative strengths of the diffuse interstellar bands in some interstellar dust clouds

, 1986
Some of the diffuse interstellar features (DIBs) in the spectra of certain stars at high galactic latitudes (1 is greater than 15 degrees) are unusually weak or absent while others have the strength expected for their color excess.
Walker, G. A. H., Krelowski, J.
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Notes Toward a Meteorology of the Cloud

, 2015
The premise of detailed forecasts is meteorological observation. An ominous cloud has eclipsed the global horizon of neoliberal capitalist realism. Researching cloud formations, I queried Google with the search term “clouds.” However, when using the term
Vredenburg, Elliot
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