c iv
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e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Long term variability of the
coronal and post – coronal
regionsof the Oe star
HD 149757 (ζ Oph)
Antoniou, A.1, Danezis, E.1, Lyratzi, E.1, Nikolaidis, D.1, Popović, L. Č.2 &
Dimitrijević, M. S.2
1. University of Athens, Faculty of Physics, Department of
Astrophysics, Astronomy and Mechanics, Panepistimioupoli,
Zographou 157 84,Athens – Greece.
2. Astronomical Observatory, Volgina 7, 11160 Belgrade,
Serbia.
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
C IV N IV N Vλ 1548.155 Åλ 1550.774 Å
λ 1238.821 Åλ 1242.804 Å
λ 1718.80 Å
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Vrot, Vrad, Vrand: Constant with time
Rotational Velocities:a component: 1400 km/sb component: 950 km/sRadial Velocities:a component: -800 km/s b component: -700 km/sRandom Velocities:a component: 320 km/s b component: 90 km/s
C IV regions
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Column Density (CD) in 1010 cm-2 of each one of the C IV resonance lines for the independent density regions of matter which create the satellite components.
λ 1548.155 Åa component: 2.15×1010 cm-2
b component: 0.72×1010 cm-2
λ 1550.774 Åa component: 1.98×1010 cm-2
b component: 0.66×1010 cm-2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
N IV region
GR methodVrad, Vrand, CD: Constant with time
Radial Velocities: -47 km/s
Random Velocities: 262 km/s
Column Density: 1.09×1010 cm-2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
N V regions
GR methodVrad, Vrand: Constant with time
Radial Velocities:a component: -1138 km/s b component: -1374 km/sc component: -1450 km/s
Random Velocities:a component: 797 km/s b component: 152 km/sc component: 71 km/s
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Column Density (CD) in 1010 cm-2 of each one of the N V resonance lines for the independent density regions of matter which create the satellite components.
λ 1238.821 Åa component: 1.13×1010 cm-2
b component: 0.25×1010 cm-2
c component: 0.07×1010 cm-
2
λ 1242.804 Åa component: 1.03×1010 cm-2
b component: 0.23×1010 cm-2
c component: 0.06×1010 cm-
2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
A statistical study of physical
parameters of the C IV density regions in 20 Oe
stars Antoniou, A.1,
Danezis, E.1, Lyratzi, E.1, Nikolaidis, D.1, Popović, L. Č.2 &
Dimitrijević, M. S.2
1. University of Athens, Faculty of Physics,
Department of Astrophysics, Astronomy and Mechanics,
Panepistimioupoli, Zographou 157 84,
Athens – Greece.2. Astronomical Observatory, Volgina 7, 11160 Belgrade,
Serbia.
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Rotational Velocities:a component: 1458 km/sb component: 821 km/sc component: 251 km/sd component: 133 km/s e component: 65 km/s
Radial Velocities:a component: -2066 km/sb component: -1743 km/sc component: -1235 km/s d component: -469 km/s e component: -80 km/s
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Random Velocities:a component: 187 km/sb component: 163 km/sc component: 130 km/sd component: 108 km/s e component: 56 km/s
FWHM:a component: 13.0 Åb component: 6.2 Åc component: 2.2 Åd component: 1.2 Å e component: 0.4 Å
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Absorbed Energy (E)
λ 1238.821 Åa component: 5.18 eVb component: 3.21 eVc component: 1.39 eVd component: 0.53 eVe component: 0.24 eV
λ 1242.804 Åa component: 4.76 eVb component: 2.85eVc component: 1.26 eVd component: 0.48 eV e component: 0.22 eV
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Column Density (CD)
λ 1238.821 Åa component: 5.65 ×1010 cm-2
b component: 4.58 ×1010 cm-2
c component: 3.65 ×1010 cm-2
d component: 2.62 ×1010 cm-2
e component: 1.17 ×1010 cm-2
λ 1242.804 Åa component: 5.54 ×1010 cm-2
b component: 4.39 ×1010 cm-2
c component: 3.56 ×1010 cm-2
d component: 2.56 ×1010 cm-2
e component: 1.17 ×1010 cm-2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
The N IV region in the spectra of 20 Oe stars
Antoniou, A.1, Danezis, E.1, Lyratzi, E.1, Nikolaidis, D.1, Popović, L. Č.2 &
Dimitrijević, M. S.2
1. University of Athens, Faculty of Physics,
Department of Astrophysics, Astronomy and Mechanics,
Panepistimioupoli, Zographou 157 84,
Athens – Greece.2. Astronomical Observatory, Volgina 7, 11160 Belgrade,
Serbia.
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Two levels of Vrad, Vrand, FWHM
Radial VelocitiesFirst level: -350 and -150 km/sSecond level: -70 km/sRandom VelocitiesFirst level: 350 and 220 km/sSecond level: 150 and 50 km/sFWHMFirst level: 5 and 3 ǺSecond level: 2 and 1 km/s Ǻ
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Two levels of Absorbed Energy and Column Density
Absorbed Energy (E)First level: 2 and 1.2 eVSecond level: 0.6 and 0.4 eV
Column Density (CD)First level: 4.5×1010 cm-2 and
3×1010 cm-2 Second level: 2.5×1010 cm-2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Investigation of the post coronal density regions
of Oe stars,through the N V UV resonance
lines Antoniou, A.1,
Danezis, E.1, Lyratzi, E.1, Nikolaidis, D.1, Popović, L. Č.2 &
Dimitrijević, M. S.2
1. University of Athens, Faculty of Physics,
Department of Astrophysics, Astronomy and Mechanics,
Panepistimioupoli, Zographou 157 84,
Athens – Greece.2. Astronomical Observatory, Volgina 7, 11160 Belgrade,
Serbia.
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Vrot: 1st level: 1800 and 1100 km/s2nd level: 400 and 200 km/s
Vrad:1st level: -2300 and -1500 km/s2nd level: -500 and -100 km/s
Vrand: 1st level: 400 and 200 km/s2nd level: 150 and 80 km/s
FWHM: 1st level: 18 and 10 Å
2nd level: 6 and 2 Å
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Two levels of Absorbed Energy (E)
λ 1238.821 ÅFirst level: 7 and 3 eVSecond level: 1 and 0.5 eV
λ 1242.804 ÅFirst level: 6.3 and 2.7 eVSecond level: 0.9 and 0.45 eV
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Two levels of Column Density (CD)
λ 1238.821 ÅFirst level:5×1010 cm-2 and 3×1010 cm-2 Second level: 2.5×1010 cm-2
λ 1242.804 ÅFirst level: 4.45×1010 cm-2 and
2.7×1010 cm-2 Second level: 2×1010 cm-2
e-mail: [email protected] [email protected]://www.cc.uoa.gr/fasma
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and MechanicsAstronomical Observatory of Belgrade
Thank you!!!