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The Rotational Behavior of Intermediate-mass F, G and K Evolved Stars Luciano Luiz Alencar de Oliveira 11/12/2014 Nata – RN Universidade Federal do Rio Grande do Norte Programa de Pós-Graduação em Física Departamento de Física Teórica e da Terra - DFTE

The rotational bahvior of intermediate mass f g-and_k envolved stars

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Page 1: The rotational bahvior of intermediate mass f g-and_k envolved stars

The Rotational Behavior of Intermediate-mass F, G and K Evolved Stars

Luciano Luiz Alencar de Oliveira 11/12/2014

Nata – RN

Universidade Federal do Rio Grande do Norte Programa de Pós-Graduação em Física

Departamento de Física Teórica e da Terra - DFTE

Page 2: The rotational bahvior of intermediate mass f g-and_k envolved stars

Objective To understand the behavior of the rotation of

intermediate mass evolved stars, such as F, G

and K.

A comparative study of the rotation of binary

and single evolved stars.

An Analysis of the infrared emission in binary

and single evolved.

Page 3: The rotational bahvior of intermediate mass f g-and_k envolved stars

Reference Data (lists of stars used in this work)

VizieR online Data Catalog: RV and vsini of evolveld

stars (de Medeiros+, 1999).

A catalog of rotational and radial velocities for evolved

stars II and Ib supergiants stars (de Medeiros+, 2002).

A catalog of rotational and radial velocities for evolved

stars: RV and vsini of southern stars (de Medeiros+,

2014)

Post annotation Extended Hipparcos Compilation

(XHIP) (Anderson+, 2012)

Page 4: The rotational bahvior of intermediate mass f g-and_k envolved stars

Luminosity Class and Spectral Type

Luminosity class are organized as follows:

Ib (supergiants)

II (bright giant)

Binary and Single

Taking the following data: parallax; distance (parsecs),

absoluta magnitude, log 𝑇𝑒𝑓𝑓, log𝐿

𝐿𝑠𝑜𝑙 e etc.

Page 5: The rotational bahvior of intermediate mass f g-and_k envolved stars

HR Diagram

Luminosity Class and Spectral Type

Page 6: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation Single Ib e II Binary Ib e II

Page 7: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 8: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 9: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 10: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 11: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 12: The rotational bahvior of intermediate mass f g-and_k envolved stars

v sin i Rotation

HR Diagram with (B-V) > 0,7

Page 13: The rotational bahvior of intermediate mass f g-and_k envolved stars

Infrared (IRAS)

Method applied by Waters et al. (1987), to normal stars:

𝑉 − 12 = 0.05 + 3.13 𝐵 − 𝑉 − 1.26 𝐵 − 𝑉 2 + 0.29 𝐵 − 𝑉 3 + 0.16 𝐵 − 𝑉 4

From of magnitudes 12, 25 e 60 µm, according to

Oudmaijer et al (1992)

𝑚𝜆 = 2.5𝑙𝑜𝑔𝐾𝜆𝑓𝜐[0.00𝑚𝑎𝑔]

𝑓𝜐

Flux density in Jy

41.04; 90.49 e 1.57

Page 14: The rotational bahvior of intermediate mass f g-and_k envolved stars

Infrared (IRAS) Binary Ib

Page 15: The rotational bahvior of intermediate mass f g-and_k envolved stars

Infrared (IRAS) Binary II

Page 16: The rotational bahvior of intermediate mass f g-and_k envolved stars

Infrared (IRAS) Single Ib

Page 17: The rotational bahvior of intermediate mass f g-and_k envolved stars

Infrared (IRAS) Single II

Page 18: The rotational bahvior of intermediate mass f g-and_k envolved stars

Orientador: Prof. Dr. José Renan de Medeiros Discente: Luciano Luiz Alencar de Oliveira E-mail: [email protected]