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19992026
most citedMass Loss: Its Effect on the Evolution and Fate of High-Mass Stars

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Showing 2005Show all

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astro-ph2005★ 11 cited

B and I-band optical micro-variability observations of the BL Lac objects S5 2007+777 and 3C371

E. M. Xilouris, I. E. Papadakis, P. Boumis +5

We have observed S5 2007+777 and 3C371 in the B and I bands for 13 and 8 nights, respectively, during various observing runs in 2001, 2002 and 2004. The observations resulted in al…

astro-ph2005★ 89 cited

Infrared [Fe II] emission from P Cygni's nebula: Atomic data, mass, kinematics, and the 1600 A.D. outburst

Nathan Smith, Patrick Hartigan

We present moderate and high-dispersion 1-2.5 micron spectra of the 10 arcsec nebula around P Cygni, dominated by bright emission lines of [Fe II]. Observed [Fe II] line ratios dis…

astro-ph2005★ 26 cited

The reverse shock of SNR1987A at 18 years after outburst

Nathan Smith, Svetozar A. Zhekov, Kevin Heng +3

We use low-dispersion spectra obtained at the Magellan Observatory to study the broad H-alpha emission from the reverse shock of the infant supernova remnant SNR1987A. These spectr…

astro-ph2005★ 15 cited

The [O III] Veil: Astropause of Eta Carinae's Wind?

Nathan Smith, Jon A. Morse, John Bally

We present narrowband images of eta Carinae in the light of [O III] 5007 obtained with HST/WFPC2, as well as a ground-based image in the same emission line with a larger field of v…

astro-ph2005★ 75 cited

Thermal Dust Emission from Proplyds, Unresolved Disks, and Shocks in the Orion Nebula

Nathan Smith, John Bally, Ralph Y. Shuping +2

We present a new 11.7 micron mosaic image of the Orion nebula obtained with T-ReCS on Gemini South. The map includes the BN/KL region, the Trapezium, and OMC-1 South. Excluding BN/…

astro-ph2005★ 26 cited

Kinematic Structure of H2 and [Fe II] in the Bipolar Planetary Nebula M 2-9

Nathan Smith, Bruce Balick, Robert D. Gehrz

We present high-dispersion long-slit IR spectra of the double-shell bipolar planetary nebula M 2-9 in the emission lines [Fe II] 16435 and H2 v=1--0 S(1) 21218. H2 spectra reveal f…