49 citations · 147 across the 6 of their papers we have counts for
6 papers
Spitzer 24 um Images of Planetary Nebulae
Y. -H. Chu, R. A. Gruendl, M. A. Guerrero +9
Spitzer MIPS 24 um images were obtained for 36 Galactic planetary nebulae (PNe) whose central stars are hot white dwarfs (WDs) or pre-WDs with effective temperatures of ~100,000 K…
Deep optical observations of the interaction of the SS 433 microquasar jet with the W 50 radio continuum shell
P. Boumis, J. Meaburn, J. Alikakos +6
Four mosaics of deep, continuum-subtracted, CCD images have been obtained over the extensive galactic radio continuum shell, W 50, which surrounds the remarkable stellar system SS…
Discovery of an M8.5 Dwarf With Proper Motion mu=2.38 arcsec/yr
Sebastien Lepine, R. Michael Rich, James D. Neill +2
We report the discovery of LSR1826+3014, a very faint (V=19.36) star with a very large proper motion (mu=2.38 arcsec/yr). A low resolution red spectrum reveals that LSR1826+3014 is…
The First Orbital Period for a Dwarf Nova in a Globular Cluster: V101 in M5
James D. Neill, Michael M. Shara, Adeline Caulet +1
We report the first orbital period determination for a Dwarf Nova (DN) in a glubular cluster: V101 in M5 has a period of 5.796 +- 0.036 hours. We derived this period from I-band ph…
Emission-Line Properties of the LMC Bubble N70
Brooke P. Skelton, William H. Waller, Richard F. Gelderman +4
We present a spectrophotometric imaging study of the emission bubble N70 (DEM 301) in the Large Magellanic Cloud. N70 is approximately 100 pc in size with a nearly circular shell-l…
Detection of Pre-Shock Dense Circumstellar Material of SN 1978K
You-Hua Chu, Adeline Caulet, Marcos Montes +3
The supernova SN 1978K has been noted for its lack of emission lines broader than a few thousand km/s since its discovery in 1990. Modeling of the radio spectrum of the peculiar SN…