We review the observational characteristics of classical and recurrent novae in the optical region, in the context of observational programmes carried out using telescopes at the Vainu Bappu Observatory (VBO) and the Indian Astronomical Observatory (IAO) of the Indian Institute of Astrophysics. The article discusses the different classes of novae, based on either their outburst light curve properties, or their spectral development. Also provided is a brief discussion on the quiescence properties of novae
Recurrent novae (RNe) belong to the group of cataclysmic variables that exhibit nova outbursts at in...
We briefly review the current theoretical understanding of the light curves of novae. These curves e...
Novae are the observable outcome of a transient thermonuclear runaway on the surface of an accreting...
Abstract. We review the observational characteristics of classical and recurrent no-vae in the optic...
Novae are interacting binary star systems consisting of a Roche-lobe filling secondary on or near th...
We describe the observable characteristics of classical novae and recurrent novae obtained by differ...
Novae are certainly very exciting at the time of their eruptions, and there is much work left to be ...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
Classical novae are transient astronomical events resulting from an eruption on the surface of an ac...
Spectroscopic and photometric behaviour of the class of recurrent novae with giant secondaries (T Co...
© 2018 The Author(s). We have monitored the return to quiescence of novae previously observed in out...
Recurrent novae (RNe) belong to the group of cataclysmic variables that exhibit nova outbursts at in...
Classical and Recurrent novae (CNe/RNe) are interacting close binary systems in which mass is transf...
Recurrent novae (RNe) belong to the group of cataclysmic variables that exhibit nova outbursts at in...
We briefly review the current theoretical understanding of the light curves of novae. These curves e...
Novae are the observable outcome of a transient thermonuclear runaway on the surface of an accreting...
Abstract. We review the observational characteristics of classical and recurrent no-vae in the optic...
Novae are interacting binary star systems consisting of a Roche-lobe filling secondary on or near th...
We describe the observable characteristics of classical novae and recurrent novae obtained by differ...
Novae are certainly very exciting at the time of their eruptions, and there is much work left to be ...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
The outbursts of classical novae are among the strongest explosions in the Universe. The multifreque...
Classical novae are transient astronomical events resulting from an eruption on the surface of an ac...
Spectroscopic and photometric behaviour of the class of recurrent novae with giant secondaries (T Co...
© 2018 The Author(s). We have monitored the return to quiescence of novae previously observed in out...
Recurrent novae (RNe) belong to the group of cataclysmic variables that exhibit nova outbursts at in...
Classical and Recurrent novae (CNe/RNe) are interacting close binary systems in which mass is transf...
Recurrent novae (RNe) belong to the group of cataclysmic variables that exhibit nova outbursts at in...
We briefly review the current theoretical understanding of the light curves of novae. These curves e...
Novae are the observable outcome of a transient thermonuclear runaway on the surface of an accreting...
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