Citation: R. Sankrit et al., Far Ultraviolet Spectroscopic Explorer observations of an x-ray bright region in the Vela supernova remnant, ASTROPHYS J, 549(1), 2001, pp. 416-424
Authors:
Sahnow, DJ
Moos, HW
Ake, TB
Andersen, J
Andersson, BG
Andre, M
Artis, D
Berman, AF
Blair, WP
Brownsberger, KR
Calvani, HM
Chayer, P
Conard, SJ
Feldman, PD
Friedman, SD
Fullerton, AW
Gaines, GA
Gawne, WC
Green, JC
Gummin, MA
Jennings, TB
Joyce, JB
Kaiser, ME
Kruk, JW
Lindler, DJ
Massa, D
Murphy, EM
Oegerle, WR
Ohl, RG
Roberts, BA
Romelfanger, ML
Roth, KC
Sankrit, R
Sembach, KR
Shelton, RL
Siegmund, OHW
Silva, CJ
Sonneborn, G
Vaclavik, SR
Weaver, HA
Wilkinson, E
Citation: Dj. Sahnow et al., On-orbit performance of the Far Ultraviolet Spectroscopic Explorer satellite, ASTROPHYS J, 538(1), 2000, pp. L7-L11
Authors:
Jenkins, EB
Oegerle, WR
Gry, C
Vallerga, J
Sembach, KR
Shelton, RL
Ferlet, R
Vidal-Madjar, A
York, DG
Linsky, JL
Roth, KC
Dupree, AK
Edelstein, J
Citation: Eb. Jenkins et al., The ionization of the local interstellar medium as revealed by Far Ultraviolet Spectroscopic Explorer observations of N, O, and Ar toward white dwarfstars, ASTROPHYS J, 538(1), 2000, pp. L81-L85
Authors:
Cox, DP
Shelton, RL
Maciejewski, W
Smith, RK
Plewa, T
Pawl, A
Rozyczka, M
Citation: Dp. Cox et al., Modeling W44 as a supernova remnant in a density gradient with a partiallyformed dense shell and thermal conduction in the hot interior. I. The analytical model, ASTROPHYS J, 524(1), 1999, pp. 179-191
Authors:
Shelton, RL
Cox, DP
Maciejewski, W
Smith, RK
Plewa, T
Pawl, A
Rozyczka, M
Citation: Rl. Shelton et al., Modeling W44 as a supernova remnant in a density gradient, with a partially formed dense shell and thermal conduction in the hot interior. II. The hydrodynamic models, ASTROPHYS J, 524(1), 1999, pp. 192-212
Citation: Rl. Shelton, Simulations of supernova remnants in diffuse media. II. Three remnants andtheir X-ray emission, ASTROPHYS J, 521(1), 1999, pp. 217-233
Citation: Rl. Shelton, Simulations of supernova remnants in diffuse media and their application to the lower halo of the Milky Way. I. The high-stage ions, ASTROPHYS J, 504(2), 1998, pp. 785-804