Interstellar dust
From interstellar dust to comets: the extended CO source in comet Halley
... refractory interstellar dust grain mantles studied by laboratory analog methods appear to provide a reasonable match to the stoichiometric distribution of the elements ob- served in comet Halley dust ...
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Comet Halley - A carrier of interstellar dust chemical evolution
... of interstellar dust has been studied by theoretical interpretation combining remote observations and laboratory experiments ...of Interstellar atoms and molecules ...
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The formation of peptide-like molecules on interstellar dust grains
... Ligterink et al. (2017, 2018). In short, it consists of a central chamber at ultra-high vacuum conditions (P ≤ 10 −10 mbar). A gold-coated, reflective surface is positioned at the center of the chamber, which is ...
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X-ray spectroscopy of interstellar dust: from the laboratory to the Galaxy
... the dust grains along the line of ...the dust grains along the line of sight, as well as the chemical composition of the ...the dust halo has an arcminute-scale maximum angular ...the dust ...
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Amorphous organic solids as a component of interstellar dust
... in interstellar clouds as well as the diffuse interstellar ...diffuse interstellar bands, the 217 nm feature, the extended red emission, the 21 and 30 μm emission features, could also arise from ...
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Filtering of the interstellar dust flow near the heliopause: the importance of secondary electron emission for the grain charging
... of interstellar dust near the ...on interstellar dust near the ...of interstellar dust in the magnetic field near the ...
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Interstellar dust close to the Sun
... Interstellar dust enters the heliosphere region at the rel- ative speed of the solar system and the ...the interstellar field and their trajectories follow that field as it is distorted by the ...the ...
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Interstellar dust within the life cycle of the interstellar medium
... of interstellar dust has made tremendous progress these last few decades, mostly thanks to infrared spectrometer and spectro-imager onboard space-born missions and thanks to the experimental effort ...
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Attempt to detect diamagnetic anisotropy of dust sized crystal orientated to investigate the origin of interstellar dust alignment
... between interstellar polarization and dust temperature was confirmed for 14 lines of sight towards the Pleiades cluster (Matsumura et ...of dust materials (Uyeda et ...
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SHOCK PROCESSING OF INTERSTELLAR DUST AND POLYCYCLIC AROMATIC HYDROCARBONS IN THE SUPERNOVA REMNANT N132D
... heated dust and/or line emission from ion- ized oxygen caused by hard photons from the remnant; it cannot solely be explained by the wider MIPS PSF (see point source in ...shocked, ...
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Costantini, Elisa (2004): Scattering and Absorption of X-rays by Interstellar Dust. Dissertation, LMU München: Fakultät für Physik
... HKJMX CVEGF q vJ <w dETFlLOLNdlSIXgFldgfFWZWCVQ?¦MFWLNwMp@/CZ\[eA ^3FdgFlFWA CVE[$CP7Q?CVEGQNA Fl[]Z5E FWbGRMF]S9CEGF. []^GdgJMXfTCQOJMA ZlXgJMdddFWZWCVQNJMA bTFlZlXgF\[]dgFzP7QN[r] ...
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Supernova Remnants as a Probe of Dust Grains in the Interstellar Medium
... cold dust in Cas A based on SCUBA (sub-mm) observations, although these conclusions have been called into question (Dwek 2004a,b; Krause et ...K) dust. A SN blast wave sweeps up gas and dust as it ...
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Evolution of dust grain size distribution by shattering in the interstellar medium: Robustness and uncertainty
... Considering that shattering is a unique mechanism that produces small grains efficiently in the ISM, it is important to clarify how robust or uncertain the theoretical calcula- tions of shattering are. Since there are ...
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Interstellar grains: Effect of inclusions on extinction
... the interstellar medium, carbon and silicate oc- cur separately and in the form of small particles which ag- glomerate into large ...composite interstellar dust, see Mathis (1996) and Vaidya et ...
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ISO-SWS spectroscopy of dust in the diffuse interstellar medium toward Cygnus OB2 no.12
... The 2.85È3.75 km region of our highest resolution SWS spectrum of Cyg OB2 No. 12 is illustrated in Figure 4. This spectral region contains the wavelengths of OÈH stretching resonances in water ice and the CÈH stretching ...
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The dust properties and physical conditions of the interstellar medium in the LMC massive star-forming complex N11
... the interstellar dust ...the dust emission in the LMC by Meixner et ...LMC dust grains have a different (larger) intrinsic submm opacity compared to mod- els which assume graphitic properties ...
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Studies of dust and gas in the interstellar medium of the Milky Way
... that dust grains are mainly composed of two chem- ically different type of species: silicates and carbonaceous materials (Zubko et ...the dust grains in the diffuse ISM have been well studied, dust ...
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The Science with the Interstellar Heliopause Probe
... While the Voyager spacecraft provide certain direct in- formation about the plasma environment in the outer helio- sphere, none is available regarding the neutral gas, and none will be available beyond about 130–140 AU, ...
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Searches for Interstellar HCCSH and H_2CCS
... by interstellar standards ) are perhaps improbable as substantial reservoirs of gas-phase sulfur, given the generally lower abundance of large molecules relative to simpler species ( see, ...
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Ashes to Ashes, Dust to Dust
... Iserson, Kenneth V., M.D. Death to Dust: What Happens to Dead Bodies? 2nd ed. 1994. Tucson: Iserson, 2001. Print. Somewhat of an encyclopedia of the Mortuary world. The author is a Professor of Emergency Medicine ...
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