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[PDF] Top 20 O VI in the Local Interstellar Medium

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O VI in the Local Interstellar Medium

O VI in the Local Interstellar Medium

... report the results of a search for O vi absorption in the spectra of 80 hot DA white dwarfs observed by the FUSE ...of the radial velocities of interstellar and ... Voir le document complet

26

The Helium Focusing Cone of the Local Interstellar Medium Close to the Sun

The Helium Focusing Cone of the Local Interstellar Medium Close to the Sun

... months. The detector, which was stored in dry nitrogen between measurement updates, has shown a 30% loss of quantum efficiency at ...over the 67 months. Admittedly, the environment experienced ... Voir le document complet

12

OVI in the local interstellar medium: FUSE observations towards B-stars within 200 pc

OVI in the local interstellar medium: FUSE observations towards B-stars within 200 pc

... which the OVI is though to form (Cox & Helenius 2003 ...for the boundary wall to the LC, thus supporting the idea of an internally high magnetic pressure (Andersson & Potter 2006 ...of ... Voir le document complet

9

Spallation-dominated propagation of heavy cosmic rays and the Local Interstellar Medium (LISM)

Spallation-dominated propagation of heavy cosmic rays and the Local Interstellar Medium (LISM)

... unlike the latter, they are not very sensitive to a source ...extract the di ffusion coef- ficient without too much ...that the heavier the nucleus, the more local it is, so that ... Voir le document complet

14

Physical processes in the interstellar medium of the Magellanic Clouds

Physical processes in the interstellar medium of the Magellanic Clouds

... within the Cycle 0 12 CO(2-1) map ( Indebetouw et ...magnitudes. The Cycle 0 map already showed that the molecular gas is clumpy in 30Dor, even with the coarser resolution of band 6 ... Voir le document complet

251

Physical conditions of the interstellar medium in high-redshift submillimetre bright galaxies

Physical conditions of the interstellar medium in high-redshift submillimetre bright galaxies

... 2 O emission in the Herschel- ATLAS 1 ( Eales et ...characterise the far-infrared radiation field generated by intense star-forming ac- tivity, and possibly AGN, and learn the physical ... Voir le document complet

175

Models of turbulent dissipation regions in the diffuse interstellar medium

Models of turbulent dissipation regions in the diffuse interstellar medium

... Both the observed abundances of CH + and column densi- ties of rotationally excited H 2 suggest that large amounts of suprathermal energy are deposited in the cold diffuse ...energy in ... Voir le document complet

23

Observations of the Interplanetary Hydrogen during Solar Cycles 23 and 24. What can We Deduce about the Local Interstellar Medium?

Observations of the Interplanetary Hydrogen during Solar Cycles 23 and 24. What can We Deduce about the Local Interstellar Medium?

... shows the IPH velocities obtained from observations by SWAN and STIS. In order to show the solar cycle effect and the influence of LISM, we overplotted the predictions from the ... Voir le document complet

7

The ALMA-PILS survey: First detection of nitrous acid (HONO) in the interstellar medium

The ALMA-PILS survey: First detection of nitrous acid (HONO) in the interstellar medium

... participate in the formation of more complex ...2 O, and HNO have been detected in the interstellar ...report the first interstellar de- tection of nitrous acid ... Voir le document complet

10

Toward the Comprehension of the Infrared to Submillimeter View of the Interstellar Medium of Nearby Galaxies

Toward the Comprehension of the Infrared to Submillimeter View of the Interstellar Medium of Nearby Galaxies

... with the Spitzer telescope as part of the SAGE (Surveying the Agents of Galaxy Evolution) project (Meixner et ...2006). The observing strategy and the data analysis of the ... Voir le document complet

205

CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium

CO excitation of normal star-forming galaxies out to z = 1.5 as regulated by the properties of their interstellar medium

... for local spirals and dynam- ically derived α CO for local ULIRGS, while for BzK galaxies they are derived by concordant estimates based on CO lumi- nosities and dust mass ...for the substantial ... Voir le document complet

20

The nearby interstellar medium toward α Leo. UV observations and modeling of a warm cloud within hot gas

The nearby interstellar medium toward α Leo. UV observations and modeling of a warm cloud within hot gas

... to the flow that is im- pacting the heliosphere ( Möbius et ...). The Therefore our Component 1, which deviates by only ...from the expectation of the model, is identified as the ... Voir le document complet

19

Are Wolf-Rayet Stars Able to Pollute the Interstellar Medium of Galaxies? Results from Integral Field Spectroscopy

Are Wolf-Rayet Stars Able to Pollute the Interstellar Medium of Galaxies? Results from Integral Field Spectroscopy

... As the local N pollution has not been observed in all the studied objects in this work and in those where it was observed, it does not show a perfect match with the ... Voir le document complet

17

High-resolution observations of interstellar Na I and Ca II towards the southern opening of the ‘Local Interstellar Chimney’: probing the disc—halo connection

High-resolution observations of interstellar Na I and Ca II towards the southern opening of the ‘Local Interstellar Chimney’: probing the disc—halo connection

... of interstellar Ca II and Na I absorption lines towards seven stars in the direction of the southern opening of the recently identified Local Interstellar ...probe ... Voir le document complet

12

Cosmic-ray propagation in the bi-stable interstellar medium. I. Conditions for cosmic-ray trapping

Cosmic-ray propagation in the bi-stable interstellar medium. I. Conditions for cosmic-ray trapping

... for local enhancements of the CR pressure, which might then change the gas dynamics in the environment of these ...sources. In addition, the initial Alfvénic Mach number ... Voir le document complet

19

Clumpiness of the interstellar medium in the central parsec of the Galaxy from H2 flux-extinction correlation

Clumpiness of the interstellar medium in the central parsec of the Galaxy from H2 flux-extinction correlation

... points in the correlation plot, as if there were no global correlation, but instead several local ...to the curve are assigned to that group and colored with a tag color. The result of ... Voir le document complet

9

The Sun's journey through the local interstellar medium: the paleoLISM and paleoheliosphere

The Sun's journey through the local interstellar medium: the paleoLISM and paleoheliosphere

... of the Local Bubble plasma pressure, the large contrast (> 10 3 ) between neutral ISM densities in the Lo- cal Bubble versus the CLIC must have generated signifi- cant changes ... Voir le document complet

10

Polarization Measurements of Hot Dust Stars and the Local Interstellar Medium

Polarization Measurements of Hot Dust Stars and the Local Interstellar Medium

... For the A stars we find that the degree of green polarization is weaker in the hot dust stars at the ...for the controls ...that the hot dust stars in this group are ... Voir le document complet

11

Helium abundance in giant planets and the local interstellar medium Helium abundance in giant planets and the local interstellar medium

Helium abundance in giant planets and the local interstellar medium Helium abundance in giant planets and the local interstellar medium

... For the protosolar nebula, the sun’s photosphere is usually used to derive the He ...oscillation, the present-day He abundance in the sun’s photosphere is derived as Yphotosphere ... Voir le document complet

13

Three-dimensional simulations of turbulent spectra in the local interstellar medium

Three-dimensional simulations of turbulent spectra in the local interstellar medium

... explore the dynamics of multiple scale coupling in a super-Alfv´enic, supersonic, and a strongly magnetized compressible MHD ...energy in shear Alfv´enic and fast/slow magne- tosonic modes (MHD ... Voir le document complet

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