Interferometric Angular Diameters of Mira Variables with theHubble Space Telescope

1997 ◽  
Vol 485 (1) ◽  
pp. 328-332 ◽  
Author(s):  
Mario G. Lattanzi ◽  
Ulisse Munari ◽  
Patricia A. Whitelock ◽  
Michael W. Feast
Keyword(s):  
Space Telescope ◽  
Mira Variables ◽  
Angular Diameters

Results from the PTI's studies of the spectral angular diameters of Mira variables

2003 ◽  
Author(s):  
Robert R. Thompson ◽  
Michelle J. Creech-Eakman ◽  
Gerard T. van Belle
Keyword(s):  
Mira Variables ◽  
Angular Diameters

scholarly journals Hubble Space Telescope Observations of Mira Variables in the SN Ia Host NGC 1559: An Alternative Candle to Measure the Hubble Constant

2020 ◽  
Vol 889 (1) ◽  
pp. 5 ◽  
Author(s):  
Caroline D. Huang ◽  
Adam G. Riess ◽  
Wenlong Yuan ◽  
Lucas M. Macri ◽  
Nadia L. Zakamska ◽  
...  
Keyword(s):  
Hubble Space Telescope ◽  
Hubble Constant ◽  
Space Telescope ◽  
Mira Variables

The Atmosphere of Mira Variables: A View with theHubble Space Telescope

2000 ◽  
Vol 536 (2) ◽  
pp. 923-933 ◽  
Author(s):  
Donald G. Luttermoser
Keyword(s):  
Space Telescope ◽  
Mira Variables

Introduction to the Solar Space Telescope

2000 ◽  
Vol 179 ◽  
pp. 141-147
Author(s):  
G. Ai ◽  
S. Jin ◽  
S. Wang ◽  
B. Ye ◽  
S. Yang
Keyword(s):  
Solar Telescope ◽  
Basic Aspect ◽  
Space Telescope ◽  
Space Solar Telescope

AbstractThe design of the space solar telescope (SST) (phase B) has been completed. The manufacturing is under development. At the end of 2000, it will be assembled. The basic aspect will be introduced in this paper.

Polarimetric Observations of Red Variables: A Study of Gas and Particle Interactions

1979 ◽  
Vol 46 ◽  
pp. 386-408 ◽  
Author(s):  
G. V. Coyne ◽  
I. S. McLean
Keyword(s):  
Wavelength Dependence ◽  
Stellar Atmosphere ◽  
Molecular Absorption ◽  
Absorption Bands ◽  
Absorption And Emission ◽  
Mira Variables ◽  
Stellar Photosphere ◽  
Regular Variable ◽  
Red Supergiants ◽  
Balmer Lines

AbstractIn recent years the wavelength, dependence of the polarization in a number of Mira variables, semi-regular variables and red supergiants has been measured with resolutions between 0.3 and 300 A over the range 3300 to 11000 A. Variations are seen across molecular absorption bands, especially TiO bands, and across atomic absorption and emission lines, especially the Balmer lines. In most cases one can ignore or it is possible to eliminate the effects due to interstellar polarization, so that one can study the polarization mechanisms operating in the stellar atmosphere and environment. The stars Omicron Ceti. (Mira), V CVn (semi-regular variable) and Mu Cephei (M2 la), in addition to other stars similar to them, will be discussed in some detail.Models to explain the observed polarization consider that the continuum flux is polarized either by electron, molecular and/or grain scattering or by temperature variations and/or geometrical asymmetries over the stellar photosphere. This polarized radiation is affected by atomic and molecular absorption and emission processes at various geometric depths in the stellar atmosphere and envelope. High resolution spectropolarimetry promises, therefore, to be a power-rul tool for studying stratification effects in these stars.

The MOLspheres of Mira Variables

2015 ◽  
Vol 71-72 ◽  
pp. 249-250
Author(s):  
K.H. Hinkle ◽  
T. Lebzelter
Keyword(s):  
Mira Variables
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