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Refinado por: Nome da Publicação: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY remover
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1
UV upturn versus UV weak galaxies differences and similarities of their stellar populations unveiled by a de-biased sample
UV upturn versus UV weak galaxies differences and similarities of their stellar populations unveiled by a de-biased sample
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UV upturn versus UV weak galaxies differences and similarities of their stellar populations unveiled by a de-biased sample

M L L Dantas Paula R. T Coelho; P Sánchez-Blásquez

Monthly Notices of the Royal Astronomical Society Oxford: Oxford University Press (OUP), 2020 h v. 500, n. 2, p. 1870–1883, 2020

Oxford 2020

Item não circula. Consulte sua biblioteca.(Acessar)

2
Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
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Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA

Ryan Leaman Paula Rodrigues Teixeira Coelho

Monthly Notices of the Royal Astronomical Society Oxford v. 488, n. 3, p. 3904-3928, 2019

Oxford 2019

Item não circula. Consulte sua biblioteca.(Acessar)

3
Time Inference with MUSE in Extragalactic Rings (TIMER) properties of the survey and high-level data products
Time Inference with MUSE in Extragalactic Rings (TIMER) properties of the survey and high-level data products
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Time Inference with MUSE in Extragalactic Rings (TIMER) properties of the survey and high-level data products

Dimitri A Gadotti Paula Rodrigues Teixeira Coelho

Monthly Notices of the Royal Astronomical Society Oxford v. 482, n. 1, p. 506-529, 2019

Oxford 2019

Item não circula. Consulte sua biblioteca.(Acessar)

4
Clocking the formation of today’s largest galaxies wide field integral spectroscopy of brightest cluster galaxies and their surroundings
Clocking the formation of today’s largest galaxies wide field integral spectroscopy of brightest cluster galaxies and their surroundings
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Clocking the formation of today’s largest galaxies wide field integral spectroscopy of brightest cluster galaxies and their surroundings

Louise O. V Edwards Paula Rodrigues Teixeira Coelho

Monthly Notices of the Royal Astronomical Society Oxford v. 491, n. 3, p. 2617-2638, 2020

Oxford 2020

Item não circula. Consulte sua biblioteca.(Acessar)

5
Testing stellar population fitting ingredients with Globular Clusters I Stellar libraries
Testing stellar population fitting ingredients with Globular Clusters I Stellar libraries
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Testing stellar population fitting ingredients with Globular Clusters I Stellar libraries

Lucimara P Martins Ciria Lima-Dias; Paula Rodrigues Teixeira Coelho; Tatiana F Lagana

Monthly Notices of the Royal Astronomical Society Oxford v. 484, n. 2, p. 2388-2402, 2019

Oxford 2019

Item não circula. Consulte sua biblioteca.(Acessar)

6
Clocking the assembly of double-barred galaxies with the MUSE TIMER project
Clocking the assembly of double-barred galaxies with the MUSE TIMER project
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Clocking the assembly of double-barred galaxies with the MUSE TIMER project

Adriana de Lorenzo-Cáceres Dimitri Alexei Gadotti; Paula Rodrigues Teixeira Coelho

Monthly Notices of the Royal Astronomical Society Oxford v. 484, n. 4, p. 5296-5314, 2019

Oxford 2019

Item não circula. Consulte sua biblioteca.(Acessar)

7
To use or not to use synthetic stellar spectra in population synthesis models?
To use or not to use synthetic stellar spectra in population synthesis models?
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To use or not to use synthetic stellar spectra in population synthesis models?

Paula Rodrigues Teixeira Coelho Gustavo Bruzual; T S Gonçalves; Stéphane Charlot

Monthly Notices of the Royal Astronomical Society Oxford v. 491, n.2, p.2025-2042, 2020

Oxford 2020

Item não circula. Consulte sua biblioteca.(Acessar)

8
UV bright red-sequence galaxies how do UV upturn systems evolve in redshift and stellar mass?
UV bright red-sequence galaxies how do UV upturn systems evolve in redshift and stellar mass?
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UV bright red-sequence galaxies how do UV upturn systems evolve in redshift and stellar mass?

M. L. L Dantas Paula Rodrigues Teixeira Coelho; T S Gonçalves

Monthly Notices of the Royal Astronomical Society Oxford v. 492, n.2, p. 2996-3011, 2020

Oxford 2020

Item não circula. Consulte sua biblioteca.(Acessar)

9
How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?
How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?
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How well can we determine ages and chemical abundances from spectral fitting of integrated light spectra?

Geraldo Gonçalves Paula Coelho |a Coelho, Paula R. T.; Ricardo Shiavon; Christopher Usher

Monthly Notices of the Royal Astronomical Society Oxford: Oxford University Press (OUP), 2020 v. 499, n. 2, p. 2327–2339, 2020

Oxford 2020

Item não circula. Consulte sua biblioteca.(Acessar)

10
Surface brightness fluctuation spectrum a new probe of evolved stars inunresolved stellar populations
Surface brightness fluctuation spectrum a new probe of evolved stars inunresolved stellar populations
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Surface brightness fluctuation spectrum a new probe of evolved stars inunresolved stellar populations

Martin Mitzkus C. Jakob Walcher; Martin M Roth; Paula Rodrigues Teixeira Coelho; Maria Rosa L Cioni; Gabriella Raimondo; Marina Rejkuba

Monthly Notices of the Royal Astronomical Society Oxford v. 480, n. 1, p. 629-651, 2018

Oxford 2018

Item não circula. Consulte sua biblioteca.(Acessar)

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Deste Autor:

  1. Coelho, P
  2. Dantas, M
  3. Souza, R
  4. Gonçalves, T
  5. Lima-Dias, C

Neste Assunto:

  1. Galáxias
  2. Aglomerados De Galáxias
  3. Cosmologia
  4. Populações Estelares
  5. Galáxias Elípticas

  • Realização: ABCD-USP USP   Logos de Redes Sociais: Freepik

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