Results 131 to 140 of about 4,999 (221)
ON THE SCALE HEIGHT OF PLANETARY-NEBULAE
Based on the distribution at high galactic latitudes, the local scale height of planetary nebulae is determined. We find a value of 250 +/- 50 pc, assuming an exponential disk, or 190 +/- 40 pc in case of an isothermal disk. This agrees well with the old
POTTASCH, [No Value], ZIJLSTRA, AA
core +1 more source
Nebular and auroral emission lines of [Cl III] in the optical spectra of planetary nebulae. [PDF]
Keenan FP +5 more
europepmc +1 more source
Dense circumstellar nebulae in wide binary central stars
Detection of close binary central stars with periods of less than a day is now well-tested and routinely possible via photometric monitoring. For wide binary central stars with periods of weeks to years detection techniques are still in their infancy ...
Miszalski, B +7 more
core
Crystallization of stardust analogs under an electron flux atmosphere. [PDF]
Shohan RA +6 more
europepmc +1 more source
C<sub>20</sub> and nitrogen-substituted fullerenes: anharmonic IR and UV-vis spectra for astrophysical environments. [PDF]
Karri VL +3 more
europepmc +1 more source
History of individual presolar SiC grains revealed by stellar winds. [PDF]
Bajo KI +4 more
europepmc +1 more source
A search for CO+ in planetary nebulae
We have carried out a systematic search for the molecular ion CO+ in a sample of 8 protoplanetary and planetary nebulae in order to determine the origin of the unexpectedly strong HCO+ emission previously detected in these sources.
Redman, Matt P.
core
Uncovering the integral spectral characteristics of the planetary nebula ICĀ 4642. [PDF]
Mohery M +4 more
europepmc +1 more source
Information-Entropy Analysis of Stellar Evolutionary Stages with Application to FS CMa Objects. [PDF]
Zhanabaev Z, Akniyazova A, Ashimov Y.
europepmc +1 more source

