Self-@consistent determination of distances and central star parameters for a large sample of Galactic Planetary Nebulae

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Int Astron Union Symp | / 180卷 / 50期

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[1] Self-consistent determination of distances and central star parameters for a large sample of galactic Planetary Nebulae
Malkov, YF
PLANETARY NEBULAE, 1997, (180): : 50 - 50
[2] A self-consistent determination of the distances, physical parameters, and chemical composition for a large sample of galactic planetary nebulae: The distances and parameters of central stars and the optical depths of envelopes
Mal'kov, YF
ASTRONOMY REPORTS, 1997, 41 (06) : 760 - 776
[3] A self-consistent determination of distances, physical parameters, and chemical composition for a large sample of galactic planetary nebulae: Chemical composition
Mal'kov, YF
ASTRONOMY REPORTS, 1998, 42 (03) : 293 - 306
[4] The central stars parameters and the distances to galactic planetary nebulae
Sharova, OI
PLANETARY NEBULAE: THEIR EVOLUTION AND ROLE IN THE UNIVERSE, 2003, (209): : 57 - 57
[5] Abundances for a large sample of Galactic planetary nebulae
Golovaty, VV
Malkov, YF
PLANETARY NEBULAE, 1997, (180): : 408 - 408
[6] GALACTIC KINEMATICS OF PLANETARY NEBULAE WITH [WC] CENTRAL STAR
Pena, Miriam
Rechy-Garcia, Jackeline S.
Garcia-Rojas, Jorge
REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA, 2013, 49 (01) : 87 - 99
[7] Distances of galactic planetary nebulae based on a relationship between the central star mass and the N/O abundance
Cazetta, JO
Maciel, WJ
REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA, 2000, 36 (01) : 3 - 11
[8] Gravity distances of planetary nebulae II. Application to a sample of galactic objects
Cazetta, JO
Maciel, WJ
ASTROPHYSICS AND SPACE SCIENCE, 2001, 277 (03) : 393 - 401
[9] Gravity Distances of Planetary Nebulae II. Application to a Sample of Galactic Objects
J.O. Cazetta
W.J. Maciel
Astrophysics and Space Science, 2001, 277 : 393 - 401
[10] ALPHA ELEMENT ABUNDANCES IN A LARGE SAMPLE OF GALACTIC PLANETARY NEBULAE
Milingo, J. B.
Kwitter, K. B.
Henry, R. B. C.
Souza, S. P.
ASTROPHYSICAL JOURNAL, 2010, 711 (02): : 619 - 630

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