To be or not to be asymmetric? VLTI and the mass loss geometry of red giants

Paladini, C.; Klotz, D.; Sacuto, S.; Wittkowski, M.; Lagadec, E.; Olofsson, H.; Groenewegen, M.; Verhoelst, T.; Richichi, A.; Jorissen, A.; Hron, J.; Kerschbaum, F.

doi:10.1117/12.926380

To be or not to be asymmetric? VLTI and the mass loss geometry of red giants - Paladini, C. et al - published in Optical and Infrared Interferometry III, 8445, pp. 84451R (2012) - ASTROimport-937

People who viewed this page also viewed:

(127) Optical and radiometric models of the NOMAD instrument part II: the infrared channels - SO and LNO - Thomas, I. R. et al - published in Optics Express, 24 issue 4, pp. 3790-3805 (2016) - SCART-2017-0027

(124) Imaging the solar corona in the EUV - Delaboudiniere, J.-P. et al - published in Advances in Space Research, 20, pp. 2231--2237 (1997) - SIDCimport-100

(123) EIT Observations of the Extreme Ultraviolet Sun - Moses, D. et al - published in Solar Physics, 175, pp. 571-599 (1997) - SIDCimport-67

(123) The qualification campaign of the EUI instrument of Solar Orbiter - Halain, Jean-Philippe et al - published in Proc. SPIE, 9905 issue Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 99052X (July 18, 2016) (2016) - SCART-2016-0009

(123) SILSO News - Clette, F. - SIDCimport-1611

Similar records

guest :: login Space Pole Publications Server
		Search		Submit		Personalize Your alerts Your baskets Your searches		Help