Citation: Eg. Blackman et Gb. Field, How astrophysical mean field dynamos can circumvent existing quenching constraints, PHYS PLASMA, 8(5), 2001, pp. 2407-2414
Citation: Sa. Hartnoll et Eg. Blackman, Reprocessed emission line profiles from dense clouds in geometrically thick accretion engines, M NOT R AST, 324(1), 2001, pp. 257-266
Citation: Eg. Blackman, Implications of mean field accretion disc theory for vorticity and magnetic field growth, M NOT R AST, 323(2), 2001, pp. 497-505
Authors:
Blackman, EG
Frank, A
Markiel, JA
Thomas, JH
Van Horn, HM
Citation: Eg. Blackman et al., Dynamos in asymptotic-giant-branch stars as the origin of magnetic fields shaping planetary nebulae, NATURE, 409(6819), 2001, pp. 485-487
Citation: Sa. Hartnoll et Eg. Blackman, Reprocessed emission from warped accretion discs with application to X-rayiron line profiles, M NOT R AST, 317(4), 2000, pp. 880-892
Citation: Eg. Blackman et Gb. Field, Resolution of an ambiguity in dynamo theory and its consequences for back-reaction studies, ASTROPHYS J, 521(2), 1999, pp. 597-601
Authors:
Herrnstein, JR
Moran, JM
Greenhill, LJ
Blackman, EG
Diamond, PJ
Citation: Jr. Herrnstein et al., Polarimetric observations of the masers in NGC 4258: An upper limit on thelarge-scale magnetic field 0.2 Parsecs from the central engine, ASTROPHYS J, 508(1), 1998, pp. 243-247