Multi-wavelength interferometry of evolved stars using VLTI and VLBA

We report on our project of coordinated VLTI/VLBA observations of the atmospheres and circumstellar environments of evolved stars. We illustrate in general the potential of interferometric measurement

References(33)

Figures(0)

[1]

VINCI-VLTI measurements of HR 4049: The Physical size of the circumbinary envelope

Simone Antoniucci
(
)
,
Francesco Paresce
(
- European Southern Observ.
)
,
Markus Wittkowski
(
- European Southern Observ.
)

- Astron.Astrophys. 429 (2005) L1-L4
•
e-Print:
- astro-ph/0411136
•
DOI:
- 10.1051/0004-6361:200400097

[2]

&P. H. Hauschildt : ADS

J.P. Aufdenberg

- Proc.SPIE Int.Soc.Opt.Eng. 4838 (2003) 193

[3]

&A. J. Kemball : ADS

D.A. Boboltz
,
P.J. Diamond

- Astrophys.J. 487 (1997) L147

[4]

&P. J. Diamond : ADS

D.A. Boboltz

- Astron.Astrophys.Suppl.Ser. 197 (2000) 4507

[5]

Joint VLBA/VLTI observations of the Mira variable S Orionis

- Astrophys.J. 618 (2005) 953-961
•
e-Print:
- astro-ph/0410232
•
DOI:
- 10.1086/426107

[6]

ADS

W.D. Cotton
,
B. Mennesson
,
P.J. Diamond

- Astron.Astrophys. 414 (2004) 275

[7]

ADS

W.C. Danchi
,
M. Bester
,
C.G. Degiacomi

- Astron.J. 107 (1994) 1469

[8]

A Movie of a star: Multi-epoch VLBA imaging of the SiO masers towards the Mira variable TX Cam

Philip J. Diamond
(
- Jodrell Bank
)
,
A.J. Kemball
(
- NRAO, Socorro
)

- Astrophys.J. 599 (2003) 1372-1382
•
e-Print:
- astro-ph/0310684
•
DOI:
- 10.1086/379347

[9]

The K-band intensity profile of R Leonis probed by VLTI/VINCI

Davide Fedele
(
- European Southern Observ. and
- Padua U., Astron. Dept.
)
,
M. Wittkowski
(
- European Southern Observ.
)
,
F. Paresce
(
- European Southern Observ.
)
,
M. Scholz
(
- Heidelberg U. and
- Sydney U.
)
,
P.R. Wood
(
- Res. Sch. Astron. Astrophys., Weston Creek
)

et al.

- Astron.Astrophys. 431 (2005) 1019
•
e-Print:
- astro-ph/0411133
•
DOI:
- 10.1051/0004-6361:20042013

[10]

ADS

A.R. Hajian
,
J.T. Armstrong
,
C.A. Hummel

- Astrophys.J. 496 (1998) 484

[11]

ADS

R. Hanbury Brown

- Mon.Not.Roy.Astron.Soc. 167 (1973) 475

[12]

&P. G. Tuthill : ADS

C.A. Haniff
,
M. Scholz

- Mon.Not.Roy.Astron.Soc. 276 (1995) 640

[13]

The NEXTGEN Model Atmosphere Grid. 2. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 K

- Astrophys.J. 525 (1999) 871-880
•
e-Print:
- astro-ph/9907194
•
DOI:
- 10.1086/307954

[14]

ADS

K.-H. Hofmann
,
M. Scholz
,
P.R. Wood

- Astron.Astrophys. 339 (1998) 846

[15]

Observations of mira stars with the IOTA/FLUOR interferometer and comparison with Mira star models

et al.

- New Astron. 7 (2002) 9
•
e-Print:
- astro-ph/0206406
•
DOI:
- 10.1016/S1384-1076(01)00085-9

[16]

Numerical simulations of stellar sio maser variability. investigation of the effect of shocks

et al.

- Astron.Astrophys. 386 (2002) 256
•
e-Print:
- astro-ph/0202426
•
DOI:
- 10.1051/0004-6361:20020202

[17]

&P. R. Wood : ADS

M.J. Ireland
,
M. Scholz

- Mon.Not.Roy.Astron.Soc. 352 (2004) 318

[18]

&S. G. Kleinmann : ADS

M. Jura

- Astrophys.J.Suppl. 73 (1990) 769

[19]

&P. J. Diamond : ADS

A.J. Kemball

- Astrophys.J. 481 (1997) L111

[20]

Kuurcz CD-ROM No. 17., Cambridge, Mass

R. Kurucz

[21]

The last gasps of vy cma: aperture synthesis and adaptive optics imagery

et al.

- Astrophys.J. 512 (1999) 351
•
e-Print:
- astro-ph/9810024
•
DOI:
- 10.1086/306761

[22]

ADS

K. Ohnaka
,
J. Bergeat
,
T. Driebe

- Astron.Astrophys. 429 (2005) 1057

[23]

ADS

A. Quirrenbach
,
D. Mozurkewich
,
D.F. Buscher

- Astron.Astrophys. 312 (1996) 160

[24]

Mira science with interferometry: A Review

Michael Scholz
(
- Heidelberg U. and
- Sydney U.
)

- Proc.SPIE Int.Soc.Opt.Eng. 4838 (2003) 163
•
e-Print:
- astro-ph/0409555
•
DOI:
- 10.1117/12.456978

[25]

Optical and near - IR spectra of O-rich Mira variables: A Comparison between models and observations

Anandmayee Tej
(
- Strasbourg Observ.
)
,
A. Lancon
(
- Strasbourg Observ.
)
,
M. Scholz
(
- Heidelberg U. and
- Sydney U.
)
,
P.R. Wood
(
- Res. Sch. Astron. Astrophys., Weston Creek
)

- Astron.Astrophys. 412 (2003) 481-494
•
e-Print:
- astro-ph/0309689
•
DOI:
- 10.1051/0004-6361:20031430

1-25 of 33
1
2
25 / page