2005A&A...433..127M


Query : 2005A&A...433..127M

2005A&A...433..127M - Astronomy and Astrophysics, volume 433127-135 (2005/4-1)

An estimate of the time variation of the abundance gradient from planetary nebulae. II. Comparison with open clusters, Cepheids and young objects.

MACIEL W.J., LAGO L.G. and COSTA R.D.D.

Abstract (from CDS):

The temporal behaviour of the radial abundance gradients has important consequences for models of the chemical evolution of the Galaxy. We present a comparison of the time variation of the abundance gradients in the Milky Way disk as determined from a sample of planetary nebulae, open clusters, cepheids and young objects, such as stars in OB associations and HII regions. We conclude that the [Fe/H] gradients as measured in open cluster stars strongly support the time flattening of the abundance gradient as determined from O/H and S/H measurements in planetary nebulae. This conclusion is also supported by the cepheid variables, for which very accurate gradients and ages can be determined, and also by some recent estimates for OB stars and HII regions. It is estimated that the average flattening rate for the last 8Gyr is in the range 0.005-0.010dex/kpc/Gyr.

Abstract Copyright: ∼

Journal keyword(s): planetary nebulae: general - ISM: abundances - Galaxy: abundances - open clusters and associations: general - Galaxy: disk

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 Cl Berkeley 29 OpC 06 53 03.6 +16 55 24   14.3       ~ 187 0

Query : 2005A&A...433..127M

Basic data :
Cl Berkeley 29 -- Open Cluster
Other object types:
otypes_help
OpC (2013A&A), Cl* (2020A&A,Cl,...), G (MCG,UGC,...)
ICRS coord. (ep=J2000) :
06 53 03.6 +16 55 24 (Optical) [ ] E 2023A&A...674A..37G
FK4 coord. (ep=B1950 eq=1950) :
06 50 10.0 +16 59 08 [ ]
Gal coord. (ep=J2000) :
197.9520 +07.9761 [ ]
Proper motions mas/yr :
0.151 -1.010 [0.021 0.025 90] C 2020A&A...633A..99C
Radial velocity / Redshift / cz :
V(km/s) 25.8 [0.3] / z(spectroscopic) 0.000086 [0.000001] / cz 25.80 [0.30]
   (Opt) A 2021A&A...651A..84M
Parallaxes (mas):
0.023 [0.012] C 2020A&A...633A..99C
Morphological type:
S: D ~
Angular size (arcmin):
6.0 6.0 0 (~) D 2010A&A...516A...3K
Fluxes (1) :
B 14.3 [~] E ~
SIMBAD within arcmin
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 362
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Identifiers (8) :
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Cl Berkeley 29 MCG+03-18-002 UZC J065303.7+165544 Z 0650.2+1659
C 0650+169 UGC 3583 Z 85-13 [KPS2012] MWSC 1008

References (187 between 1850 and 2026) (Total 187)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Velocities : 9    Distance : 6    Fe/H : 11    Plx : 6    PM : 9   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : Cl Berkeley 29

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UGC 3583

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