User profiles for P. Eggleton

Paul Eggleton

- Verified email at nhm.ac.uk - Cited by 20077

Paul Eggleton

- Verified email at exeter.ac.uk - Cited by 8393

[HTML][HTML] Calreticulin: non-endoplasmic reticulum functions in physiology and disease

LI Gold, P Eggleton, MT Sweetwyne… - The FASEB …, 2010 - ncbi.nlm.nih.gov
Calreticulin (CRT), when localized to the endoplasmic reticulum (ER), has important functions
in directing proper conformation of proteins and glycoproteins, as well as in homeostatic …

The ins and outs of calreticulin: from the ER lumen to the extracellular space

S Johnson, M Michalak, M Opas, P Eggleton - Trends in cell biology, 2001 - cell.com
Calreticulin was first isolated 26 years ago. Since its discovery as a minor Ca 2+ -binding
protein of the sarcoplasmic reticulum, the appreciation of its importance has grown, and it is …

Establishing the evidence base for maintaining biodiversity and ecosystem function in the oil palm landscapes of South East Asia

…, GR Broad, AYC Chung, P Eggleton… - … of the Royal …, 2011 - royalsocietypublishing.org
The conversion of natural forest to oil palm plantation is a major current threat to the conservation
of biodiversity in South East Asia. Most animal taxa decrease in both species richness …

The evolution of low mass stars

PP Eggleton - Monthly Notices of the Royal Astronomical …, 1971 - academic.oup.com
This paper presents a method of computing the evolution of low mass stars from the main
sequence to the helium flash. Many such computations are handicapped by the fact that the …

Approximations to the radii of Roche lobes

PP Eggleton - … 1 (ISSN 0004-637X), vol. 268, May 1, 1983, p …, 1983 - adsabs.harvard.edu
… If a star just fills its Roche lobe, its mean density p (g cm-3) is related to the orbital period
P (days) by … Hence, P(p)1/2 is a function of q only, which we can approximate via …

The equilibrium tide model for tidal friction

PP Eggleton, LG Kiseleva, P Hut - The Astrophysical Journal, 1998 - iopscience.iop.org
We derive from first principles the equations governing (a) the quadrupole tensor of a star
distorted both by rotation and by the presence of a companion in a possibly eccentric orbit;(b) …

Composition changes during stellar evolution

PP Eggleton - Monthly Notices of the Royal Astronomical …, 1972 - academic.oup.com
This paper presents an algorithm by means of which composition changes in stars due to
nuclear reactions, convection and semiconvection can be relatively simply calculated. The …

Biodiversity inventories, indicator taxa and effects of habitat modification in tropical forest

…, DE Bignell, B Bolton, GF Bloemers, P Eggleton… - Nature, 1998 - nature.com
Despite concern about the effects of tropical forest disturbance and clearance on biodiversity
1 , 2 , data on impacts, particularly on invertebrates, remain scarce 3 , 4 , 5 , 6 , 7 , 8 . Here …

[BOOK][B] Evolutionary processes in binary and multiple stars

P Eggleton - 2006 - books.google.com
… The coefficients are to be found in Eggleton et al. (1973). A second virtue of the above …
Since much of the physics we need involves derivatives of p, S wrt T,ρ, it is important that the …

Approximate input physics for stellar modelling

OR Pols, CA Tout, PP Eggleton… - Monthly Notices of the …, 1995 - academic.oup.com
We present a simple and efficient, yet reasonably accurate, equation of state, which at the
moderately low temperatures and high densities found in the interiors of stars less massive …