Repository landing page

We are not able to resolve this OAI Identifier to the repository landing page. If you are the repository manager for this record, please head to the Dashboard and adjust the settings.

Study of nova shells. I. V1229 Aquilae (1970) : nebular expansion parallax and luminosity

Abstract

The maximum magnitude - rate of decline (MMRD) relation of classical novae is briefly reviewed, and attention is drawn on superluminous and subluminous novae. Such objects play an important role when the MMRD relation is applied to small or magnitude-limited samples of novae. Direct imaging tance, reddening and luminosity are derived. With MV = -6.7, V1229 Aql is 1m fainter than predicted by the MMRD

Similar works

This paper was published in OA@INAF - Istituto Nazionale di Astrofisica.

Having an issue?

Is data on this page outdated, violates copyrights or anything else? Report the problem now and we will take corresponding actions after reviewing your request.