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This ESA Herschel image shows IRC10216 also known as CW

This ESA Herschel image shows IRC10216 also known as CW

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This ESA Herschel image shows IRC+10216, also known as CW Leonis, a

This Herschel image shows IRC+10216, also known as CW Leonis - a star rich in carbon where astronomers were surprised to find water.

... In combined data from ESA's Herschel and NASA's Spitzer telescopes, irregular distribution of dust in ...

... This image from ESA's Herschel Space Observatory reveals a suspected ring at the center of our ...

... The dark hole seen in the green cloud at the top of this image, captured; This ESA Herschel image shows IRC+10216, also known as CW ...

Fig. A.1. SPIRE 250 μ m image of IRC + 10216 after

... The large bubble is an embryonic star that looks set to turn into one of the ...

Some of the coldest and darkest dust in space shines brightly in this infrared image from

Figure 1. ExPo image of the circumstellar environment of IRC + 10216 in polarised intensity

... This parallelogram shaped region of dust observed by ESA's Herschel Space telescope can be best described ...

... This image from NASA's Herschel, in the constellation of Vulpecula, shows an entire assembly ...

Comparison between PACS images and deconvolved VLT / FORS1 V -band image (see Fig

A Herschel study of NGC 650

This ESA Herschel image shows IRC+10216, also known as CW Leonis, a star rich in carbon where astronomers were surprised to find water. | Pinterest

... This map shows the distribution of water in the stratosphere of Jupiter as measured with the

The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology

PACS 100 μ m image (in units of mJy / arcsec 2 ) of IRC

Mean intensity enhancements (in Jy / arcsec 2 ) in each sector of

Imaging Planetary Nebulae with Herschel-PACS and SPIRE

Zoom into the inner 5 30

Herschel -PACS scan maps ( left to right : at 70

X Herculis and TX Piscium: Two cases of ISM interaction with stellar winds observed by Herschel

The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology

Illustration of water-producing processes around a carbon star

This ESA Herschel image shows IRC+10216, also known as CW Leonis, a star rich in carbon where astronomers were surprised to find water. | Pinterest

X Herculis and TX Piscium: Two cases of ISM interaction with stellar winds observed by Herschel

Fig. 2. Two views of the filamentary structure of the Musca cloud showing the

Radial Surface brightness profiles in the five Herschel bands for the original

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vlt-omega-nebula-desk-1680.jpg ...

Imaging Planetary Nebulae with Herschel-PACS and SPIRE

Image

Relative line strength of some water vapor lines as observed with Herschel/PACS in the bright carbon sources IRC +10216, V Hya, CIT 6, and V Cyg.

Fig. 3.-Calculated abundances of Mg-bearing species in IRC +10216

Observed expansion velocity for different molecular lines observed with Herschel/HIFI in a sample of oxygen-rich AGB stars (Justtanont et al., 2012).

X Herculis and TX Piscium: Two cases of ISM interaction with stellar winds observed by Herschel

Herschel Probes the Dusty History of a Giant Star

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Download full-size image

Imaging Planetary Nebulae with Herschel-PACS and SPIRE

Fig. 6 Maps of the emission in the 101 GHz lines of CH 3 OH

Herschel/PACS observations of OH127.8+0.0 (black) compared to model predictions. Both a model with a low dust-to-gas ratio [Math Processing Error] ψ of ...

The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology

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Figure 1. Observed spectrum of IRC+10216 in B configuration. It contains lines

Fig. 14. Fits to the 69 μm band of forsterite using temperature dependent opacities (de Vries et al., 2011). Fits are shown for the post-AGB star HD 161796 ...

The Herschel Exploitation of Local Galaxy Andromeda (HELGA). I: Global far-infrared and sub-mm morphology

heic0918a-globular-cluster-desk-1024.jpg ...

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Fig. 1. Pointing of H-and V-polarisation beams. The beam

Figure 2. Grey-scale representations (top panel) of the line profile variations

hubble-ultradeep-desk-1800.jpg ...

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... This image from the Herschel Observatory, a European Space Agency mission, reveals some of ...

Contrast enhanced deconvolved Herschel-PACS 70 μm image of W

Това изображение показва увеличения изглед на една от петте галактики, открити от Хершел. Галактиката е кръстена SDP 81 и е жълтата точка в лявото ...

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Comparison between the rich Herschel/PACS spectra of the O-rich AGB star R Dor (black), the O-rich supergiant VY CMa (gray) and the C-rich AGB star CIT 6 ...

iceberg-b15a-apr2005-desk-1024.jpg ...

Fig. 3. PHT22 ISO-PHOT observation of AQ And. A red circle

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The color image shows the spectral index map derived from the 321

Herschel observations of planetary nebulae in the MESS key program

Fig. 1. Coralie spectrum of BH Cru, smoothed to a resolution of ∼

mars-mera-columbia-wideshot-desk-1800a.jpg ...

TABLE 3 LIMITING FAINT SOURCE DETECTION LIMITS (10σ IN 10,000 S) AND BRIGHT SOURCE

The main window shows the ISO-SWS spectrum of IRAS 17150

Figure 7. Picture of the 0.5U KUL ADCS, containing three reaction wheels,

Testing of the cruise stage for NASA's Mars Science Laboratory in August 2010 included a session

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Fig. 8. Upper panels: ALMA 12 CO(1–0) and

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J. Cernicharo | Research Professor | Instituto de Ciencia de Materiales de Madrid, Madrid | ICMM | Group of Molecular Astrophysics | Page 8

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Th. Posch's scientific contributions while affiliated with University of Vienna

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Fig. 4. Spectra of the H 2 O, HCO + , and HCN

Detection of the 69 {\mu}m band of crystalline forsterite in the Herschel MESS-program

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Fig. 5. Spectrum of IRC+10216 covering the J = 71−70

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Fig. 7. The SED of OH 127.8+0.0. In black the combined

Table 1 . Summary of observations at 257 GHz towards IRC+10216

Venus Spins Slower than Before

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Fig. 8. Left panel : surface brightness in comet C / 2006 W3 (

Figure 5. The spectral energy distribution of IRAS 05280−6910. The measured infrared

Fig. 3. Evolution of the flux ratio between the NE and SW images of

Figure 3. SCUBA-2 imaging of the AU Mic disk. North is up

Fig. 8. Effect of pixfrac in the PSF projection. The panels show the

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Figure 3. The atmospheric transparency at zenith between 50 and 950 GHz for 0.5 mm