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On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits
On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits
Material Type:
Artículo 		Añadir a Mi Portal

On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits

J. H Groh D. J Hillier; Augusto Damineli Neto

The Astrophysical Journal Chicago v. 737, p. 46/1-46/13, 2011

Chicago 2011

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2
To v∞ and beyond! The He I absorption variability across the 2014.6 periastron passage of η Carinae
To v∞ and beyond! The He I absorption variability across the 2014.6 periastron passage of η Carinae
Material Type:
Artículo 		Añadir a Mi Portal

To v∞ and beyond! The He I absorption variability across the 2014.6 periastron passage of η Carinae

Noel D Richardson Thomas Madura; Lucas St-Jean; Anthony F. J Moffat; Theodore R Gull; Christopher M. P Russell; Augusto Damineli Neto; Mairan Teodoro; Michael F Corcoran; Frederick M Walter; Nicola Clementel; Jose H Groh; Kenji Hamaguchi; D. John Hillier

Oxford v. 461, p. 2540-2558, 2016 Monthty Notices of the Royal Astronomical Society

Oxford 2016

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3
On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits
On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits
Material Type:
Artículo 		Añadir a Mi Portal

On the nature of the prototype luminous blue variable A G Carinae II. Witnessing a massive star evolving close to the Eddington and bistability limits

J. H Groh D. J Hillier; Augusto Damineli Neto

The Astrophysical Journal Chicago v. 737, p. 46/1-46/13, 2011

Chicago 2011

Comprobar fondos(Obténgalo)

4
Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae
Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae
Material Type:
Artículo 		Añadir a Mi Portal

Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae

J.H Groh R Barbá; Augusto Damineli Neto; D.J Hillier Fernández-Lajús; R. C Gamen; A. P Moisés; G Solivella; M Teodoro

The Astrophysical Journal Chicago v. 705, p. L25-L30, 2009

Chicago 2009

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5
The fossil wind structures of Eta Carinae changes across one 5.54-yr cycle
The fossil wind structures of Eta Carinae changes across one 5.54-yr cycle
Material Type:
Artículo 		Añadir a Mi Portal

The fossil wind structures of Eta Carinae changes across one 5.54-yr cycle

Theodore R Gull Thomas I Madura; Mairan Teodoro; Nicola Clementel; Michael Corcoran; Augusto Damineli Neto; Jose H Groh; Kenji Hamaguchi; D. John Hillier; Anthony F. J Moffat; Noel D Richardson; Gerd Weigelt; Don Lindler; Keith Feggans

0035-8711 Monthly Notices of the Royal Astronomical Society Oxford v. 462, p. 3196-3220, 2016

Oxford 2016

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6
Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae
Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae
Material Type:
Artículo 		Añadir a Mi Portal

Bona fide, strong-variable galactic luminous blue variable stars are fast rotators detection of a high rotational velocity in HR Carinae

J.H Groh R Barbá; Augusto Damineli Neto; D.J Hillier Fernández-Lajús; R. C Gamen; A. P Moisés; G Solivella; M Teodoro

The Astrophysical Journal Chicago v. 705, p. L25-L30, 2009

Chicago 2009

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  1. Atmosferas Estelares  (5)
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por este autor/creador:

  1. Damineli Neto, A
  2. Groh, J
  3. Hillier, D
  4. Teodoro, M
  5. Moffat, A

con este tema:

  1. Estrelas Variáveis
  2. Perda De Massa
  3. Atmosferas Estelares
  4. Estrelas
  5. Estrelas Binárias

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