Correlation between N/O nebular ratio and central star mass: distances to galactic PN (1997)
Source: Planetary Nebulae: proceedings. Conference titles: International Astronomical Union Symposium. Unidade: IAG
Assunto: ASTRONOMIA
ABNT
CAZETTA, J O e MACIEL, Walter Junqueira. Correlation between N/O nebular ratio and central star mass: distances to galactic PN. 1997, Anais.. Dordrecht: Kluwer, 1997. . Acesso em: 28 mar. 2024.APA
Cazetta, J. O., & Maciel, W. J. (1997). Correlation between N/O nebular ratio and central star mass: distances to galactic PN. In Planetary Nebulae: proceedings. Dordrecht: Kluwer.NLM
Cazetta JO, Maciel WJ. Correlation between N/O nebular ratio and central star mass: distances to galactic PN. Planetary Nebulae: proceedings. 1997 ;[citado 2024 mar. 28 ]Vancouver
Cazetta JO, Maciel WJ. Correlation between N/O nebular ratio and central star mass: distances to galactic PN. Planetary Nebulae: proceedings. 1997 ;[citado 2024 mar. 28 ]