Follow
Peter Storey
Peter Storey
Emeritus Professor of Physics, UCL
Verified email at star.ucl.ac.uk
Title
Cited by
Cited by
Year
Recombination-line intensities for hydrogenic ions – I. Case B calculations for H I and He II
DG Hummer, PJ Storey
Monthly Notices of the Royal Astronomical Society 224 (3), 801-820, 1987
11721987
Recombination line intensities for hydrogenic ions-IV. Total recombination coefficients and machine-readable tables for Z= 1 to 8
PJ Storey, DG Hummer
Monthly Notices of the Royal Astronomical Society 272 (1), 41-48, 1995
10511995
Theoretical values for the [O iii] 5007/4959 line-intensity ratio and homologous cases
PJ Storey, CJ Zeippen
Monthly Notices of the Royal Astronomical Society 312 (4), 813-816, 2000
5842000
Atomic data for opacity calculations. II. Computational methods
KA Berrington, PG Burke, K Butler, MJ Seaton, PJ Storey, KT Taylor, ...
Journal of Physics B: Atomic and Molecular Physics 20 (23), 6379, 1987
5521987
NGC 6153: a super-metal-rich planetary nebula?
XW Liu, PJ Storey, MJ Barlow, IJ Danziger, M Cohen, M Bryce
Monthly Notices of the Royal Astronomical Society 312 (3), 585-628, 2000
3792000
Dielectronic recombination at low temperatures. II Recombination coefficients for lines of C, N, O
H Nussbaumer, PJ Storey
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 56, June …, 1984
292*1984
Dielectronic recombination at low temperatures
H Nussbaumer, PJ Storey
Astronomy and Astrophysics (ISSN 0004-6361), vol. 126, no. 1, Sept. 1983, p …, 1983
2841983
MOCASSIN: a fully three-dimensional Monte Carlo photoionization code
B Ercolano, MJ Barlow, PJ Storey, XW Liu
Monthly Notices of the Royal Astronomical Society 340 (4), 1136-1152, 2003
2742003
The C III transition probabilities
H Nussbaumer, PJ Storey
Astronomy and Astrophysics, vol. 64, no. 1-2, Mar. 1978, p. 139-144. 64, 139-144, 1978
2571978
The dusty mocassin: fully self-consistent 3D photoionization and dust radiative transfer models
B Ercolano, MJ Barlow, PJ Storey
Monthly Notices of the Royal Astronomical Society 362 (3), 1038-1046, 2005
2172005
Transition probabilities for forbidden Fe II infrared lines
H Nussbaumer, PJ Storey
Astronomy and Astrophysics (ISSN 0004-6361), vol. 193, no. 1-2, March 1988 …, 1988
1991988
Chemical abundances of planetary nebulae from optical recombination lines—III. The Galactic bulge PN M 1-42 and M 2-36
XW Liu, SG Luo, MJ Barlow, IJ Danziger, PJ Storey
Monthly Notices of the Royal Astronomical Society 327 (1), 141-168, 2001
1922001
The rich O II recombination spectrum of the planetary nebula NGC 7009: new observations and atomic data
XW Liu, PJ Storey, MJ Barlow, RES Clegg
Monthly Notices of the Royal Astronomical Society 272 (2), 369-388, 1995
1911995
Heavy elements in Galactic and Magellanic Cloud H ii regions: recombination-line versus forbidden-line abundances
YG Tsamis, MJ Barlow, XW Liu, IJ Danziger, PJ Storey
Monthly Notices of the Royal Astronomical Society 338 (3), 687-710, 2003
1832003
The O (2+)/H (+) abundance ratio in gaseous nebulae derived from recombination lines
M Peimbert, PJ Storey, S Torres-Peimbert
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 414, no. 2, p. 626-631 …, 1993
1671993
Atomic data from the IRON Project-LVIII. Electron impact excitation of
PJ Storey, G Del Zanna, HE Mason, CJ Zeippen
Astronomy & Astrophysics 433 (2), 717-730, 2005
146*2005
Atomic Processes and Applications
MJ Seaton, PJ Storey
North-Holland 135, 1976
1421976
C II two-electron transitions
H Nussbaumer, PJ Storey
Astronomy and Astrophysics, vol. 96, no. 1-2, Mar. 1981, p. 91-95. 96, 91-95, 1981
1411981
A deep survey of heavy element lines in planetary nebulae–I. Observations and forbidden-line densities, temperatures and abundances
YG Tsamis, MJ Barlow, XW Liu, IJ Danziger, PJ Storey
Monthly Notices of the Royal Astronomical Society 345 (1), 186-220, 2003
1402003
Recombination coefficients for O II lines at nebular temperatures and densities
PJ Storey
Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 3, p. 999-1013 …, 1994
1371994
The system can't perform the operation now. Try again later.
Articles 1–20