Tartalom
Képek
Kép feltöltése
DSS Images Other Images
Kapcsolódó cikkek
Bispectrum speckle interferometry of IRC +10216: The dynamic evolution of the innermost circumstellar environment from 1995 to 2001
We present new near-infrared (JHK) bispectrum speckle-interferometrymonitoring of the carbon star IRC+10216 obtainedbetween 1999 and 2001 with the SAO 6 m telescope. The J-, H-, and K-bandresolutions are 50 mas, 56 mas, and 73 mas, respectively. The totalsequence of K-band observations covers now 8 epochs from 1995 to 2001and shows the dynamic evolution of the inner dust shell. The presentobservations show that the appearance of the dust shell has considerablychanged compared to the epochs of 1995 to 1998. Four main componentswithin a 0\farcs2 radius can be identified in the K-band images. Theapparent separation of the two initially brightest components A and Bincreased from ~ 191 mas in 1995 to ~ 351 mas in 2001. Simultaneously,component B has been fading and almost disappeared in 2000 whereas theinitially faint components C and D became brighter (relative to peakintensity). The changes of the images can be related to changes of theoptical depth caused, for instance, by mass-loss variations or new dustcondensation in the wind. Our recent two-dimensional radiative transfermodel of IRC +10216 suggests that the observedrelative motion of components A and B is not consistent with the outflowof gas and dust at the well-known terminal wind velocity of 15 kms-1. The apparent motion with a deprojected velocity of 19 kms-1 on average and of recently 27 km s-1 appearsto be caused by a displacement of the dust density peak due to dustevaporation in the optically thicker and hotter environment. The presentmonitoring, covering more than 3 pulsation periods, shows that thestructural variations are not related to the stellar pulsation cycle ina simple way. This is consistent with the predictions of hydrodynamicalmodels that enhanced dust formation takes place on a timescale ofseveral pulsation periods. The timescale of the fading of component Bcan well be explained by the formation of new dust in the circumstellarenvelope.
| Photoelectric observations of lunar occultations. XII
Occultation observations of 414 events observed between 6 July 1979 and4 September 1980 with the 0.76-m telescope of McDonald Observatory arereported. Timings and data on double stars are given. Angular diameterinformation in six cases is included. The stars concerned with their runnumbers are: SAO 161754 (5270); 94027 (Alpha Tau) (5319, 5381, 5454);159370 (Gamma Lib) (5325, 5571); 162413 (43 Sgr) (5332); 97472 (3 Cnc)(5414); and 93955 (Theta Tau) (5445).
|
Új cikk hozzáadása
Kapcsolódó hivatkozások
- - (nincs kapcsolódó hivatkozás) -
Új link hozzáadása
Besorolás csoportokba:
|
Pozíciós és asztrometriai adatok
| Csillagkép: | Oroszlán |
| Rektaszcenzió: | 09h41m38.75s |
| Deklináció: | +12°53'55.1" |
| Vizuális fényesség: | 7.907 |
| Távolság: | 219.298 parszek |
| RA sajátmozgás: | 26.6 |
| Dec sajátmozgás: | -14.1 |
| B-T magnitude: | 9.165 |
| V-T magnitude: | 8.011 |
Katalógusok és elnevezések:
|
