Pregled bibliografske jedinice broj: 971523
Circumstellar Dust in Symbiotic Novae
Circumstellar Dust in Symbiotic Novae // The Physics of Evolved Stars / Lagadec, E. ; Millour, F. ; Lanz, T. (ur.).
Lahti: EAS Publications Series, 2015. str. 159-162 doi:10.1051/eas/1571035 (predavanje, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 971523 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Circumstellar Dust in Symbiotic Novae
Autori
Jurkić, Tomislav ; Kotnik-Karuza, Dubravka
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
The Physics of Evolved Stars
/ Lagadec, E. ; Millour, F. ; Lanz, T. - Lahti : EAS Publications Series, 2015, 159-162
ISBN
978-2-7598-1907-2
Skup
The Physics of Evolved Stars
Mjesto i datum
Nica, Francuska, 08.06.2015. - 12.06.2015
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
AGB stars, symbiotic binaries, radiative transfer, numerical modelling
Sažetak
We present a model of inner dust regions around the cool Mira component of the two symbiotic novae, RR Tel and HM Sge, based on the near-IR photometry, ISO spectra and mid-IR interferometry. The dust properties were determined using the DUSTY code. A compact circumstellar silicate dust shell with inner dust shell temperatures between 900 K and 1300 K and of moderate optical depth can explain all the observations. RR Tel shows the presence of an equatorially enhanced dust density during minimum obscuration. Obscuration events are explained by an increase in optical depth caused by the newly condensed dust. The mass loss rates are significantly higher than in intermediate-period single Miras but in agreement with longer-period O-rich AGB stars.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2014-09-8656 - Zvijezde i prašina: struktura, sastav i interakcija (STARDUST) (Pavlovski, Krešimir, HRZZ - 2014-09) ( CroRIS)
Ustanove:
Sveučilište u Rijeci - Odjel za fiziku
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)