We report the spectroscopic follow-up of the nova V459 Vul carried out at the Loiano Observatory, Italy, at three epochs after the outburst. The spectroscopy showed high ionization lines of iron. The photometry has been used to estimate the absolute magnitude at maximum and the distance of the nova. V459 Vul is a fast nova, with decline times by two and three magnitudes of 18 and 30 days respectively. The nova achieved an absolute magnitude at maximum of -8.7 ... -7.7. The distance of V459 Vul is in the range 2.3-5.0 kpc. (C) 2009 Elsevier B.V. All rights reserved
Aims: We aim to derive the physical properties of the recurrent nova T Pyx and the structure of the ...
Spectral evolution of the fast nova V1494 Aql was monitored soon after its discovery in December 199...
We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift...
We present results of the spectroscopic monitoring of the peculiar nova V458 Vul during eleven month...
We report the spectroscopic observations of nova V2670 Oph secured at the Loiano Observatory, Italy,...
We present the spectroscopy of nova V2467 Cyg acquired at the Loiano Observatory, Italy, during the ...
We report results of spectroscopic observations of V382 Vel (Nova Vel 1999) carried out at La Silla ...
We report the spectroscopic follow-up of the nova V5558 Sgr carried out in 2008 and 2009 at the Loia...
We present the optical spectral evolution of the nova V2362 Cyg during the first 15 months after the...
Context.Classical novae are quite frequent in M 31. However, very few spectra of M 31 novae have be...
We have secured optical spectroscopy of the nova V5584 Sgr at the Loiano Observatory, Italy, during ...
Spectral evolution of the fast nova V1494 Aql was monitored soon after its discovery in December 199...
We present results of our dense spectroscopic monitoring of Nova V5668 Sgr. Starting on March 19 in ...
We continue the analysis of the multiwavelength evolution of the recurrent nova T Pyx during its 201...
Our CCD photometry of Nova Scuti 2005 N.2 (=V477 Sct) shows it to be a very fast nova, which is cha...
Aims: We aim to derive the physical properties of the recurrent nova T Pyx and the structure of the ...
Spectral evolution of the fast nova V1494 Aql was monitored soon after its discovery in December 199...
We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift...
We present results of the spectroscopic monitoring of the peculiar nova V458 Vul during eleven month...
We report the spectroscopic observations of nova V2670 Oph secured at the Loiano Observatory, Italy,...
We present the spectroscopy of nova V2467 Cyg acquired at the Loiano Observatory, Italy, during the ...
We report results of spectroscopic observations of V382 Vel (Nova Vel 1999) carried out at La Silla ...
We report the spectroscopic follow-up of the nova V5558 Sgr carried out in 2008 and 2009 at the Loia...
We present the optical spectral evolution of the nova V2362 Cyg during the first 15 months after the...
Context.Classical novae are quite frequent in M 31. However, very few spectra of M 31 novae have be...
We have secured optical spectroscopy of the nova V5584 Sgr at the Loiano Observatory, Italy, during ...
Spectral evolution of the fast nova V1494 Aql was monitored soon after its discovery in December 199...
We present results of our dense spectroscopic monitoring of Nova V5668 Sgr. Starting on March 19 in ...
We continue the analysis of the multiwavelength evolution of the recurrent nova T Pyx during its 201...
Our CCD photometry of Nova Scuti 2005 N.2 (=V477 Sct) shows it to be a very fast nova, which is cha...
Aims: We aim to derive the physical properties of the recurrent nova T Pyx and the structure of the ...
Spectral evolution of the fast nova V1494 Aql was monitored soon after its discovery in December 199...
We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift...