Add to ORKGA search to find spatially resolved nova shells was carried out; two new shells (around FH Ser 1970 and V533 Her 1963) were discovered. The angular sizes measured at the current epoch of the eight previously known shells around novae which erupted prior to 1945 imply that the shells are coasting out at constant velocity. Expansion velocities, interstellar absorptions, and masses of the ejected material were determined for several recent novae. A new calibration of the maximum visual luminosity-rate of decline relationship for galactic novae is given
Following our tentative discovery of a faint shell around V1315 Aql reported in Sahman et al., we un...
The recent GAIA DR2 measurements of distances to galactic novae have allowed to re-analyse some prop...
During the last two years we have used the Palomar Testbed Interferometer to observe several explosi...
A search to find spatially resolved nova shells was carried out; two new shells (around FH Ser 1970 ...
Eight new spatially resolved nova shells have been found by imaging with a digital detector through ...
An optical imaging study of recent 30 novae has been undertaken using both ground-based and space-ba...
Nova shells can provide important information on their distance, their interactions with circumstell...
A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The m...
Nova shells are characteristically prolate with equatorial bands and polar caps. Failure to account ...
We have used data obtained with the Fine Guidance Sensors on the Hubble Space Telescope to derive pr...
The Hubble Space Telescope has imaged the central part of M87 over a 10 week span, leading to the di...
We present the results of a search for nova shells around 101 cataclysmic variables (CVs), using H α...
(abridged) Expansion distances (or expansion parallaxes) for classical novae are based on comparing ...
A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The m...
We present photometric and spectroscopic follow-up of a sample of extragalactic novae discovered by ...
Following our tentative discovery of a faint shell around V1315 Aql reported in Sahman et al., we un...
The recent GAIA DR2 measurements of distances to galactic novae have allowed to re-analyse some prop...
During the last two years we have used the Palomar Testbed Interferometer to observe several explosi...
A search to find spatially resolved nova shells was carried out; two new shells (around FH Ser 1970 ...
Eight new spatially resolved nova shells have been found by imaging with a digital detector through ...
An optical imaging study of recent 30 novae has been undertaken using both ground-based and space-ba...
Nova shells can provide important information on their distance, their interactions with circumstell...
A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The m...
Nova shells are characteristically prolate with equatorial bands and polar caps. Failure to account ...
We have used data obtained with the Fine Guidance Sensors on the Hubble Space Telescope to derive pr...
The Hubble Space Telescope has imaged the central part of M87 over a 10 week span, leading to the di...
We present the results of a search for nova shells around 101 cataclysmic variables (CVs), using H α...
(abridged) Expansion distances (or expansion parallaxes) for classical novae are based on comparing ...
A classical nova is an eruption on the surface of a white dwarf in an accreting binary system. The m...
We present photometric and spectroscopic follow-up of a sample of extragalactic novae discovered by ...
Following our tentative discovery of a faint shell around V1315 Aql reported in Sahman et al., we un...
The recent GAIA DR2 measurements of distances to galactic novae have allowed to re-analyse some prop...
During the last two years we have used the Palomar Testbed Interferometer to observe several explosi...