Sentences with phrase «for aus»

As a young adult I became a research assistant at ICI labs in the science of Dulux for Aus.

Alinta sold this wind farm to a wholly - owned subsidiary of the ANZ, Energy Infrastructure Trust, in April 2007 for Aus $ 225m.

I enrolled in this earlier today and tried to enroll online for my AU as well, but it said to call in for AUs.

No cost for additional cards for AUs.

Keep in mind that Amex requires a SSN for AUs, so it will show on credit report.

(Aus / NZ) Early name for Aus / NZ breed callend Tibetan (not to be confused with European Tibetan breed)- mitted colourpoint polydactyl of Persian / Exotic type cat.

Not exact matches

In the US one households can walk away (and this is a viable circuit breaker) but in Aus the stakes are so much higher — because the debt follows the mortgagee for life.

And always when he is in London he bring me some delicious snacks from The Mae home to Germany — soooo good To say Thank - you I made your Raw Brownies for him on his Birthday viele liebe Grüße aus Deutschland, Christina

If you're in Aus, my go - to is Farmer's Union Greek Style Yoghurt for all of the same reasons.

My organic co-op (where I get my seasonal box of vegies from) has just started stocking golden castor sugar, black - strap molasses, rapunzel stock cubes, organic mustards, and various of your other favoured ingredients, usually very hard to find here, which makes me think there's been quite a few requests for them from other Melbourne (aus) 101 readers!

I served these with toasty warm French bread loaves and a small bowl of aus jus for dipping.

After hearing rumors in Australia that there would be Aus $ 400 million cut from the National Health and Medical Research Council budget, researchers mounted a vigorous protest campaign that was successful in maintaining current spending for the major research agencies.

In addition, all three stars (including Proxima) were among the «Tier 1» target stars for NASA's optical Space Interferometry Mission (SIM) to detect a planet as small as three Earth - masses within two AUs of its host star (and so some summary system information and images on Stars A, B, and C are available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal of NASA funding.

During the relatively brief, combined giant phases of the two stars at present, however, a planet could orbit the Aab pair far enough out for the two stars to act as a single gravitational source and near enough for it to receive enough energy to sustain life, possibly around 12.5 AUs out from the binary.

According to the Astronomisches Rechen - Institut's Catalogue of Nearby Stars (ARICNS), Heintz's 1994 analysis of Mu Herculis Aa also derived an updated period of 65 years which would imply a semi-major axis of just under 17.2 AUs, assuming that the combined mass of Mu Herculis Aab is 1.2 times that of Sol's (which is consistent with Wanner's 1967 estimate of the mass ratio of 0.50 (+ / - 0.04) for the binary pair BC — combined — to the primary).

Recent numerical integrations, however, suggest that stable planetary orbits exist: within three AUs (four AUs for retrograde orbits) of either Alpha Centauri A or B in the plane of the binary's orbit; only as far as 0.23 AU for 90 - degree inclined orbits; and beyond 70 AUs for planets circling both stars (Weigert and Holman, 1997).

The two teams, led by David Koerner (of the Planetary Origins Research Group at the University of Pennsylvania) using the Owens Valley Radio Observatory and David Wilner (of the Harvard - Smithsonian Center for Astrophysics) using the Plateau de Bure Interferometer of the Institut de RadioAstronomie Millimetrique (IRAM) in the French Alps, collected millimeter - wavelength observations that were sensitive to structures as small as 20 AUs.

According to one type of model calculations performed for the NASA Star and Exoplanet Database, the inner edge of Altair's habitable zone is located relatively far from the star at around 2.177 AUs from the star, while the outer edge lies even farther out at around 4.475 AUs.

The simulations indicated that one (or more) very massive planet within 50 to 60 AUs may have destroyed the inner circumstellar dust disk by gravitational scattering (Abstract for 2002 AAS session 86.07).

Estimates provided by the NASA Star and Exoplanet Database, however, appear to be incorrect for this spectral class K star — where the inner edge of Star B's habitable zone should be located around 1.20 AU from the star, while the outer edge edge lies around 2.38 AUs, and so estimates from 40 Omicron Eridani A (another K0 - 1 star) were applied as a rough proxy, which indicated that the inner edge of Star B's habitable zone could be located around 0.56 AU from the star, while the outer edge edge lies around 1.10 AUs.

Proxima has been selected to be one of the Tier 1 target stars for NASA's Space Interferometry Mission (SIM)-- which is planned for launch as early as 2011 — to detect a planet as small as three Earth - masses within two AUs of its host star.

No Jupiter - class planets within 3 AUs were detected dusing radial - velocity variations by 2006 (Wittenmyer et al, 2006, page 186, Table 5; (Cumming et al, 1999; Abt and Levy, 1976, page 286, Table 2 for HR 799).

According to one type of model calculations performed for the NASA Star and Exoplanet Database, the inner edge of Star A's habitable zone should be located around 1.17 AU from the star, while the outer edge edge lies around 2.33 AUs.

According to one type of model calculations performed for the NASA Star and Exoplanet Database, the inner edge of 61 Vir's habitable zone should be located around 0.76 AU from the star, while the outer edge edge lies around 1.52 AUs.

Infrared excess from dust particles at 70 micrometers in size was detected at around 5 AUs out from Zeta Doradus (Trilling et al, 2008; and Bryden et al, 2006, pp. 36 and 41 for HD 33262).

According to one type of model calculations performed for the NASA Star and Exoplanet Database, the inner edge of 47 UMa's habitable zone should be located around 1.03 AUs from the star, while the outer edge edge lies around 2.06 AUs.

According to the Ninth Catalogue of Spectroscopic Binary Orbits (for HD 210027), Stars A and B move around each other at an average distance of only 0.051 AUs (semi-major axis a = 0.00407 + / - 0.27») in a highly circular (e ~ 0) orbit that takes just 10.2 days to complete.

In 2008, a search using high - contrast, infrared imaging for a planet below 10 Jupiter - masses within 25 AUs of the binary stars was negative (Bonnet - Bideaud and Pantin, 2008).

It was also selected as a «Tier 1» target star for NASA's optical Space Interferometry Mission (SIM) to detect a planet as small as three Earth - masses within two AUs of its host star (and so some summary system information and images of Epsilon Indi may still be available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal of NASA funding.

According to the Astronomiches Rechen - Institut at Heidelberg's ARICNS entry for Gl 33, BD +04 123 was once thought to have a flaring, presumably stellar companion at a separation of around 20 AUs (2.69» at 340.7 ° in 71.62 to 270» at 353.2 ° in 78.69), but Hei 202 was not be found in the reference cited (Wulff Dieter Heintz, 1985).

According to one type of model calculations performed for the NASA Star and Exoplanet Database, the inner edge of Tau Ceti's habitable zone is located relatively far from the star at around 0.582 AUs from the star, while the outer edge lies even farther out at around 1.157 AUs.

In any case at a distance of about 27.3 ly, with a period of 1.834 years and a combined mass for Aab of around 1.45 Solar - masses, the semi-major axis should be around around 1.69 AUs wide.

Infrared interferometric observations of Denebola's debris disk were used by Akeson et al (2009) to model two possible bands of dust beginning around 0.13 AU (and extending for 0.3 AUs) and around 13 AUs (extending for 6.2 AUs).

While NASA's Wide - field Infrared Survey Explorer (WISE) failed to the tell - tale warmth of gas giants like Saturn within 10,000 AUs and larger than Jupiter objects out to 26,000 AUs (NASA / JPL news release), an icy «super-Earth», would have been too cold and faint for WISE to detect — even if the hypothesized planet has a small internal heat source and absorbs some sunlight.

It was also selected as a «Tier 1» target star for NASA's optical Space Interferometry Mission (SIM) to detect a planet as small as three Earth - masses within two AUs of its host star (and so some summary system information and images of Eta Cassiopeiae A and B may still be available from the SIM Teams), but the SIM project manager announced on November 8, 2010 that the mission was indefinitely postponed due to withdrawal of NASA funding.

Hence, the minimum separation of the C component from the brighter pair is around the order of 9,000 AUs, and»... the parabolic velocity of the companion would at most be 0.7 km / sec, assuming a total mass of 2.5 for the triple system.»

(I'm in Australia, so I know the terminology can sometimes be different for certain vegetables between Aus and US).

These word are very inspiring und funny as well and above all your outfit looks so gorgeous for the occasion Lovely Week lg aus München xx

Thank you for your perfect blog — Martina aus München

I got a large in size and I'm size 10 - 12 (aus size) so it fits well for me but I am absolutely in love with these shorts, and I'm short enough that I can use these as high waisted shorts, I'm not sure if it's suppose to be or not but it totally works for me.

I hope you enjoyed fashion week, I so wish I was back in Aus for it!

Hope all is well in Aus — say hi her for me — I miss it!

Its freezing at the moment for spring here in aus, so im missing warm weather too hehe.

I opted for the UK10 (which is about an Aus size 8 - 10, US size 6).

Fritzi aus Preußen summer sandals for women.

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