... Discovering and Characterizing the Young SupernovaRemnant Population in M101 . ... Combined HST and Chnadra imaging of the supernovaremnant SNR 0509-67.5 in the LMC . ...
... 1.6 Completed FOS/BL 4108 (SupernovaRemnants and Nucleosynthesis (FOS 30): Augmentation Cycle 2) The Faint Object Spectrograph (Blue Side) was used to obtain spectral observations over the range of 1150 - 6800 A0 of SupernovaRemnant N-49 to study the ...
... Object Spectrograph was used on both the Red and Blue sides to make spectral observations of the supernovaremnant NGC-4449-SN ... FOR NEXT REPORTING PERIOD: 3.1 Complete FOS/RD 3296 (SupernovaRemnants and Nucleo Synthesis) 3.2 Complete FOS/RD 4206 ...
... 1.5 Completed FOS/RD 5680 (SupernovaRemnants and Nucleosynthesis) The FOS (Red Side) was used to obtain spectra of supernovaremnant 0504-69 in the LMC. ...
... 1.14 Completed HSP/POL 4888(Remnant Stars in SupernovaRemnants AUG - Cycle 3 High) The High Speed Photometer was used to make observations of the supernovaremnant SS443 which is known to have emission lines which vary in velocity by relativistic amounts ...
... 1.4 Completed FOS/RD 6331 (SupernovaRemnants and Nucleosynthesis (FOS = 30): Cycle 4 Aug. ... Side) was used to make = ultraviolet and optical observations of the supernovaremnant SNR = 0519-69-OP located in the Large ...
... 1.1 Completed FOS/RD 5363 (Probing the Shocked Ejecta of a Young Remnant:Cycle 4 Medium) The FOS (Red Side) was used to observe the young supernovaremnant SN1978K (V=18.7) in NGC-1313 to examine the widths, positions and fluxes of UV emission lines ...