An Optical Recombination Line Abundance Survey for Galactic Bulge Planetary Nebulae

Author(s):  
W. Wang ◽  
X.-W. Liu ◽  
Y. Zhang ◽  
Y. Liu



2009 ◽  
Vol 5 (S265) ◽  
pp. 354-355
Author(s):  
Oscar Cavichia ◽  
Roberto D. D. Costa ◽  
Walter J. Maciel

AbstractNew abundances of planetary nebulae located towards the bulge of the Galaxy are derived based on observations made at LNA (Brazil). We present accurate abundances of the elements He, N, S, O, Ar, and Ne for 56 PNe located towards the galactic bulge. The data shows a good agreement with other results in the literature, in the sense that the distribution of the abundances is similar to those works. From the statistical analysis performed, we can suggest a bulge-disk interface at 2.2 kpc for the intermediate mass population, marking therefore the outer border of the bulge and inner border of the disk.



Author(s):  
G. Stasinska ◽  
A. Acker ◽  
A. Fresneau ◽  
J. F. Gameiro ◽  
J. Köppen ◽  
...  


1993 ◽  
pp. 337-338 ◽  
Author(s):  
N. A. Walton ◽  
M. J. Barlow ◽  
R. E. S. Clegg


1989 ◽  
pp. 167-167
Author(s):  
M. W. Feast ◽  
T. D. Kinman ◽  
B. S. Lasker


2005 ◽  
Vol 157 (2) ◽  
pp. 371-395 ◽  
Author(s):  
Mark Robertson‐Tessi ◽  
Donald R. Garnett


1993 ◽  
Vol 155 ◽  
pp. 581-581 ◽  
Author(s):  
N.A. Walton ◽  
M.J. Barlow ◽  
R.E.S. Clegg

We present abundance determinations, in particular of carbon, and C/O ratios, for 11 Galactic bulge planetary nebulae (PN) based on our low resolution UV data from IUE observations and optical spectrophotometry from the Anglo-Australian Telescope. We compare the observed abundances with those predicted by dredge-up theory for the high metallicity Galactic bulge. The sample abundances are also contrasted with the abundances found for PN in the Galactic disk. The mean C/O ratio for the bulge PN is significantly lower than that found for Galactic disk PN. Further, we present an abundance analysis of the very metal-poor bulge PN M2-29. From an analysis of the differential extinction found from the observed ratios of the He ii 1640,4686Å lines, we find that the ultraviolet reddening law towards the bulge is steeper than in the solar neighbourhood.



2017 ◽  
Vol 129 (976) ◽  
pp. 067002
Author(s):  
Travis N. Stenborg


2011 ◽  
Vol 414 (2) ◽  
pp. 1667-1678 ◽  
Author(s):  
L. Guzman-Ramirez ◽  
A. A. Zijlstra ◽  
R. NíChuimín ◽  
K. Gesicki ◽  
E. Lagadec ◽  
...  


1993 ◽  
Vol 155 ◽  
pp. 573-573
Author(s):  
A.A. Nikitin ◽  
A.F. Kholtygin ◽  
A.A. Sapar ◽  
T. Kh. Feklistova

Carbon, nitrogen and oxygen abundances have been found from the recombination lines for 63 planetary nebulae.



Sign in / Sign up

Export Citation Format

Share Document