1983
DOI: 10.1093/mnras/202.3.833
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IUE and other new observations of the slow nova RR Tel

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Cited by 97 publications
(115 citation statements)
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“…Thus, in determining the distance to the star, one should take into account the fact that the extinction in the direction of the cool component includes circumstellar as well as interstellar extinction. The interstellar extinction towards RR Tel is E(B − V) = 0.10−0.11 (Penston et al 1983;Young et al 2005) which would give A K ∼ 0.03 mag.…”
Section: Distance Estimatesmentioning
confidence: 96%
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“…Thus, in determining the distance to the star, one should take into account the fact that the extinction in the direction of the cool component includes circumstellar as well as interstellar extinction. The interstellar extinction towards RR Tel is E(B − V) = 0.10−0.11 (Penston et al 1983;Young et al 2005) which would give A K ∼ 0.03 mag.…”
Section: Distance Estimatesmentioning
confidence: 96%
“…Since its nova-like optical outburst in 1944 long term spectroscopic and photometric observations have been carried out in the UV, optical and IR spectral regions in order to establish a satisfactory model of this puzzling object. Inter-comparison of data from observations in different wavelength regions made a significant contribution to these attempts (Heck & Manfroid 1985;Contini & Formiggini 1999;Penston et al 1983;Whitelock 1987).…”
Section: Introductionmentioning
confidence: 99%
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“…Although it is one of the most studied symbiotic systems, many of the physical parameters defining RR Tel are still uncertain, including the orbital period of the system. A better understanding of this system is needed in order to understand its extraordinarily diverse and rich emission line spectrum (Penston et al 1983). RR Tel is one of the few known symbiotic novae, it erupted in 1945.…”
Section: Rr Telmentioning
confidence: 99%
“…Examples can be seen in Selvelli & Bonifacio (2000) and Selvelli et al (2007). Penston et al (1983) made a thorough study of the IUE spectrum of RR Tel, where they identified more than 400 emission lines in the UV range. Harper et al (1999) used HST Goddard High Resolution Spectrograph (GHRS) spectra to provide constraints to atomic data for O IV.…”
Section: Introductionmentioning
confidence: 99%