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Ozarba nebula

 
National Institutes of Health

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2017
2017
We conduct three-dimensional hydrodynamical simulations of two opposite jets launched obliquely to the orbital plane around an… Expand
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2016
2016
NASA from Space Telescope Science Institute [GO-13469]; NASA [NAS 5-26555]; NSF [AST-0407380, AST-0909073, AST-1313370]; JPL 
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2012
2012
Several [WC]-type central stars of planetary nebulae (PNe) are known to mimic the spectroscopic appearance of massive carbon-rich… Expand
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2012
2012
Detailed observations of a recently recognized eruptive variable, V900 Mon, are presented. The star is located in the small cloud… Expand
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2012
2012
The central star of the planetary nebula PRTM 1 (PN G243.8 37.1) was previously found to be variable by M. Pe˜ na and colleagues… Expand
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2009
2009
K 3-35 is a planetary nebula (PN) where H2O maser emission has been detected, suggesting that it departed from the proto-PNe… Expand
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2005
2005
We present the results of an XMM-Newton observation of the field of the Wolf-Rayet star WR 40. Despite a nominal exposure of 20… Expand
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2001
2001
ABSTRA C T The hydrogen-deficient [WCL] type central star HD 167362 and its planetary nebula (PN) SwSt 1 are investigated. The… Expand
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1998
1998
Flux-calibrated low-resolution spectra covering the optical wavelength range from 3400 to 7500 A have been obtained over the… Expand
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1988
1988
A fast pulsar with period of 39.5 milliseconds has been discovered in the peculiar combination nebula CTB80. This nebula has been… Expand
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