Paulus-Roberge Class Reasoning Test

Roberge, James J.; Paulus, Dieter H.

doi:10.1037/t09937-000

Cited by 8 publications

(8 citation statements)

References 0 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Moreover, some clinical biochemical parameters were also disturbed by the dietary protein treatment, such as the lowered adrenal and serum DBH activities. These data are supported by the recent works of Thibault and Roberge [49,50] and Roberge and Charbonneau [19], who showed that dietary proteins selectively affect the serum DBH activity in cats adapted to different sources of protein.…”

Section: Discussionsupporting

confidence: 78%

Changes in Serum Amino Acid Content and Dopamine-β-Hydroxylase Activity and Brain Neurotransmitter Interaction in Cats Fed Casein with or without Gluten or Gliadin

Thibault

Coulon

Roberge

et al. 1988

J. Clin. Biochem. Nutr.

View full text Add to dashboard Cite

Section: Discussionsupporting

confidence: 78%

Changes in Serum Amino Acid Content and Dopamine-β-Hydroxylase Activity and Brain Neurotransmitter Interaction in Cats Fed Casein with or without Gluten or Gliadin

Thibault

Coulon

Roberge

et al. 1988

J. Clin. Biochem. Nutr.

View full text Add to dashboard Cite

“…As instrumentation improves we are likely to be able to detect debris discs to lower values of R 24 . Large Binocular Telescope Interferometer (LBTI) for example is intended to be able to detect dust at 10 μm down to a level R 10 ∼ 10 −4 (Hinz et al 2008;Roberge et al 2012). While the debris may drop below R 24 ∼ 0.1 at the times discussed in Section 4 there is still material present after this time and such a dramatic increase in sensitivity would lead to a much longer time spent above the detection threshold.…”

Section: Developments With Future Instrumentsmentioning

confidence: 99%

Debris from terrestrial planet formation: the Moon-forming collision

Jackson

Wyatt

2012

Monthly Notices of the Royal Astronomical Society

145

182

View full text Add to dashboard Cite

We study the evolution of debris created in the giant impacts expected during the final stages of terrestrial planet formation. The starting point is the debris created in a simulation of the Moon-forming impact. The dynamical evolution is followed for 10 Myr including the effects of Earth, Venus, Mars and Jupiter. The spatial distribution evolves from a clump in the first few months to an asymmetric ring for the first 10 kyr and finally becoming an axisymmetric ring by about 1 Myr after the impact. By 10 Myr after the impact 20% of the particles have been accreted onto Earth and 17% onto Venus, with 8% ejected by Jupiter and other bodies playing minor roles. However, the fate of the debris also depends strongly on how fast it is collisionally depleted, which depends on the poorly constrained size distribution of the impact debris. Assuming that the debris is made up of 30% by mass mm-cm-sized vapour condensates and 70% boulders up to 500 km, we find that the condensates deplete rapidly on ~1000 yr timescales, whereas the boulders deplete predominantly dynamically. By considering the luminosity of dust produced in collisions within the boulder-debris distribution we find that the Moon-forming impact would have been readily detectable around other stars in Spitzer 24 micron surveys for around 25 Myr after the impact, with levels of emission comparable to many known hot dust systems. The vapour condensates meanwhile produce a short-lived, optically thick, spike of emission. We use these surveys to make an estimate of the fraction of stars that form terrestrial planets, F_TPF. Since current terrestrial planet formation models invoke multiple giant impacts, the low fraction of 10-100 Myr stars found to have warm (~150 K) dust implies that F_TPF ~<10%.Comment: 23 pages, 19 figures (14 colour), 1 table. Accepted in MNRA

show abstract

“…The clitic is therefore a sort of affix, as argued by Roberge (1990) (Cummins and Roberge 1993 strengthen this hypothesis by suggesting that clitics are inflectional affixes). The clitic is therefore a sort of affix, as argued by Roberge (1990) (Cummins and Roberge 1993 strengthen this hypothesis by suggesting that clitics are inflectional affixes).…”

Section: Clitic-placement: Derivation Vs Base-generationmentioning

confidence: 86%

Pronouns in Germanic and Romance languages: An overview

Cardinaletti¹

1999

Eurotyp

View full text Add to dashboard Cite

Paulus-Roberge Class Reasoning Test

Cited by 8 publications

References 0 publications

Changes in Serum Amino Acid Content and Dopamine-β-Hydroxylase Activity and Brain Neurotransmitter Interaction in Cats Fed Casein with or without Gluten or Gliadin

Changes in Serum Amino Acid Content and Dopamine-β-Hydroxylase Activity and Brain Neurotransmitter Interaction in Cats Fed Casein with or without Gluten or Gliadin

Debris from terrestrial planet formation: the Moon-forming collision

Pronouns in Germanic and Romance languages: An overview

Contact Info

Product

Resources

About