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[PDF] Top 20 Study of the Far Infrared Emission of Nearby Spiral Galaxies

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Study of the Far Infrared Emission of Nearby Spiral Galaxies

Study of the Far Infrared Emission of Nearby Spiral Galaxies

... matter. The currently observed distribution of specific angular momentum (angular momentum per unit mass) of disk galaxies suggest very specific formation scenarios (although uncertainties ... Voir le document complet

178

LeMMINGs – I. The eMERLIN legacy survey of nearby galaxies. 1.5-GHz parsec-scale radio structures and cores

LeMMINGs – I. The eMERLIN legacy survey of nearby galaxies. 1.5-GHz parsec-scale radio structures and cores

... in the optical FPBHA, stretch- ing their luminosities up to FR I radio ...in the low-luminosity regime, the physical process which regulates the conversion of the accretion flow ... Voir le document complet

46

Modelling the ultraviolet-to-infrared spectral energy distributions of galaxies

Modelling the ultraviolet-to-infrared spectral energy distributions of galaxies

... to the SINGS sample 87 The total infrared luminosity L d tot and the stellar mass M ∗ remain reasonably well ...characteristic of Galactic cirrus emission, and if no other ... Voir le document complet

207

The far-infrared spectroscopic surveyor (FIRSS)

The far-infrared spectroscopic surveyor (FIRSS)

... external galaxies can be found in atomic, ionized or molecular state, with a range of densities and ...temperatures. The ISM can be fur- ther characterized by a few ‘phases’ depending on physical ... Voir le document complet

31

Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging

Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging

... µm) of 6.7 ′′ (11.0 ′′ ) provide a more accurate location of the dust emission than the bolometer data taken with SCUBA, AzTEC, MAMBO or ...explore the diagnostic potential ... Voir le document complet

7

The [CII] 158 μm line emission in high-redshift galaxies

The [CII] 158 μm line emission in high-redshift galaxies

... With the advent of the Atacama Large Millimeter Array (ALMA) and NOEMA, it is now possible to measure the dust content of very high redshift galaxies, but also to use ... Voir le document complet

19

Dust emission from clusters of galaxies: statistical detection

Dust emission from clusters of galaxies: statistical detection

... summed. The intensity is scaled between −50 000 to 50 000 Jy/sr for all the ...that the galaxy clusters are resolved. Neverthless the inaccuracy in the position of the ... Voir le document complet

11

Thick discs, and an outflow, of dense gas in the nuclei of nearby Seyfert galaxies

Thick discs, and an outflow, of dense gas in the nuclei of nearby Seyfert galaxies

... variety of sources and methods, Hicks et al. ( 2009 ) ar- gued that the typical gas mass fraction lies in the range 4–25 per cent, with a typical value of f gas ∼ ...within the central ... Voir le document complet

18

Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey

Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey

... gather infrared photometric data from 8 µm to 500 µm from Spitzer, WISE, IRAS, and Herschel for all of the HRS ...to the data from which the stellar contribution has been carefully ... Voir le document complet

34

A resolved analysis of cold dust and gas in the nearby edge-on spiral NGC 891

A resolved analysis of cold dust and gas in the nearby edge-on spiral NGC 891

... whether the asymmetry arises due to higher rates of star formation in the north or greater dust obscuration in the south, it is crucial to study the dust surface density and ... Voir le document complet

21

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

... 1.2.3 The ionised gas Hot ionised gas This phase is also called coronal gas or hot intercloud medium ...(HIM). The HIM shows very hot temperatures varying between 10 5 and 10 6 K and is very tenuous, with a ... Voir le document complet

205

Analysis of dust emission in nearby galaxies : implications of the modeling assumptions

Analysis of dust emission in nearby galaxies : implications of the modeling assumptions

... telescopes. The level of precision in IR observations was largely increased with the Spitzer Space Telescope ( Werner et ...at the two shortest ...µm. The spectrometer, IRS ... Voir le document complet

168

Study of $^{19} $Na at SPIRAL

Study of $^{19} $Na at SPIRAL

... p), the probability for elastic scattering changes signifi- cantly. The scattered proton can escape the target because of its smaller energy loss, and can be detected at forward angles in ... Voir le document complet

13

Study of the behavior of iron ore particles in spiral concentrators

Study of the behavior of iron ore particles in spiral concentrators

... with the 3-turn-spiral. The departure from the anticipated recovery increase is systematic and cannot be attributed solely to the problems of the feed and wash water ... Voir le document complet

118

A microbolometer-based far infrared radiometer to study thin ice clouds in the Arctic

A microbolometer-based far infrared radiometer to study thin ice clouds in the Arctic

... that the atmospheric reanalysis, the model and measurements are all consistent and of good ...2015). The high sensitivity of the simulations to specific humidity in F-IR bands ... Voir le document complet

16

Towards an Algorithmic Guide to Spiral Galaxies

Towards an Algorithmic Guide to Spiral Galaxies

... to the galaxy and is to the left or to the right of a red ...is the case, color it also ...that the row of red fields is a separator of the ...Color ... Voir le document complet

13

Added value of far-infrared radiometry for remote sensing of ice clouds

Added value of far-infrared radiometry for remote sensing of ice clouds

... investigated the potential of FIR radiometry for the characterization of ice cloud properties, with a special focus on cloud effective particle ...used the optimal estimation framework, ... Voir le document complet

24

Towards an Algorithmic Guide to Spiral Galaxies

Towards an Algorithmic Guide to Spiral Galaxies

... instance of Spiral Galaxies has a solution that contains only size-1 and size-2 ...galaxy of center g is exactly its kernel ...by the location of its center. If we assume ... Voir le document complet

24

Spiral Arms in the Disk of HD 142527 from CO Emission Lines with ALMA

Spiral Arms in the Disk of HD 142527 from CO Emission Lines with ALMA

... version of this figure is available in the online ...instead of the minus sign given in Muto et al. (2012) since the disk of HD 142527 is rotating ...fixing the values ... Voir le document complet

5

ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes

ORIGIN: Blind detection of faint emission line galaxies in MUSE datacubes

... respectively. The parameter N DCT controls the number of DCT basis vectors used in the continuum ...in the resid- ual spectrum, while a value that is too large tends to capture spectral ... Voir le document complet

15

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