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EROS variable stars: discovery of a slow nova in the SMC
Uppsala University.
Uppsala University.
Uppsala University.
Uppsala University.
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1998 (English)In: ASTRONOMY AND ASTROPHYSICS, Vol. 335, no 3, L93-L96 p.Other (Other scientific)
Abstract [en]

We report the discovery of a slow nova found in the core of the Small Magellanic Cloud by the EROS microlensing survey. Nova SMC 1994 is a classical nova with a DQ Her type lightcurve characterized by a deep minimum. Low amplitude variations occurring on

Place, publisher, year, pages
SPRINGER VERLAG , 1998. Vol. 335, no 3, L93-L96 p.
Keyword [en]
surveys; stars : novae; cataclysmic variables; galaxies : Magellanic Clouds; SPECTRAL EVOLUTION; EXTINCTION
Identifiers
URN: urn:nbn:se:uu:diva-85306OAI: oai:DiVA.org:uu-85306DiVA: diva2:113214
Note
Addresses: de Laverny P, Univ Montpellier 2, GRAAL, CC72, Pl Bataillon, F-34095 Montpellier 05, France. Astron Observ, S-75120 Uppsala, Sweden. Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands. S African Astron Observ, ZA-7925 Cape Town, South AfricAvailable from: 2008-10-17 Created: 2008-10-17

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