A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis (2017)
- Authors:
- USP affiliated authors: DIAZ, MARCOS PEREZ - IAG ; COELHO, PAULA RODRIGUES TEIXEIRA - IAG
- Unidade: IAG
- DOI: 10.3847/1538-4365/aa7681
- Assunto: ATMOSFERAS ESTELARES
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
- ISSN: 0067-0049
- Volume/Número/Paginação/Ano: v.231, n. 1, p.1, 2017
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
LEVENHAGEM, Ronaldo Savarino et al. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v. 231, n. 1, p. 1, 2017Tradução . . Disponível em: https://doi.org/10.3847/1538-4365/aa7681. Acesso em: 24 abr. 2024. -
APA
Levenhagem, R. S., Diaz, M. P., Coelho, P. R. T., & Hubeny, I. (2017). A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 231( 1), 1. doi:10.3847/1538-4365/aa7681 -
NLM
Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/aa7681 -
Vancouver
Levenhagem RS, Diaz MP, Coelho PRT, Hubeny I. A grid of synthetic spectra for hot DA white dwarfs and its application in stellar population synthesis [Internet]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES. 2017 ;231( 1): 1.[citado 2024 abr. 24 ] Available from: https://doi.org/10.3847/1538-4365/aa7681 - A new library of theoretical stellar spectra for stellar population applications
- Self-similarity in the chemical evolution of galaxies and the delay-time distribution of SNe Ia
- Surface brightness fluctuation spectrum: a new probe of evolved stars inunresolved stellar populations
- UV upturn versus UV weak galaxies: differences and similarities of their stellar populations unveiled by a de-biased sample
- Clocking the formation of today’s largest galaxies: wide field integral spectroscopy of brightest cluster galaxies and their surroundings
- To use or not to use synthetic stellar spectra in population synthesis models?
- Grids of synthetic spectra
- Biblioteca de espectros sintéticos de alta resolução, do ultravioleta ao infravermelho, com razão ['ALFA'/ Fe] variável, para síntese de populações estelares
- Abundance patterns in early-type galaxies: is there a "knee" in the [Fe/H] vs. ['alfa'/Fe] relation?
- Bar effects on ionized gas properties and dust content in galaxy centers
Informações sobre o DOI: 10.3847/1538-4365/aa7681 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
