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| V* V1391 Cas , the SIMBAD biblio (31 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:50:25 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
2021ApJ...907...70F |
1195 | T A | X C | 27 | 6 | ~ |
Transient formation of C2 and CN in the near-maximum phase of Nova Cas 2020(= V1391 Cas). |
FUJII M., ARAI A. and KAWAKITA H. | |
| 2020ATel13903....1S | 206 | T | X | 4 | 2 | ~ |
Spectroscopic classification of TCP J00114297+6611190 as classical nova. |
SOKOLOVSKY K., AYDI E., CHOMIUK L., et al. | |
| 2020ATel13904....1S | 165 | T | X | 3 | 2 | ~ |
FRAM-ORM pre-discovery photometry of the Galactic nova TCP J00114297+6611190. |
SOKOLOVSKY K., KARPOV S., MASEK M., et al. | |
| 2020ATel13905....1M | 288 | T | X | 6 | 1 | ~ |
Photometry and spectroscopy of Nova Cas 2020 ( TCP J00114297+6611190). |
MUNARI U., SIVIERO A., VAGNOZZI A., et al. | |
| 2020ATel13919....1S | 288 | T | X | 6 | 1 | ~ |
Swift observation of Nova Cassiopeiae 2020 = TCP J00114297+6611190 before peak optical brightness. |
SOKOLOVSKY K., CHOMIUK L., KAWASH A., et al. | |
| 2020ATel13939....1S | 165 | T | X | 3 | 2 | ~ |
Optical spectroscopic monitoring of Nova Cas 2020 = TCP J00114297+6611190. |
SHORE S.N., BOUSSIN C., BOYD D., et al. | |
| 2020ATel13941....1F | 206 | T | X | 4 | 3 | ~ |
Detection of molecular absorption bands of C2 and CN in Nova Cas 2020 (= TCP J00114297+6611190). |
FUJII M., ARAI A. and KAWAKITA H. | |
|
2021ApJ...912...19D |
269 | D | S X | 6 | 24 | 26 | A population of heavily reddened, optically missed novae from Palomar Gattini-IR: constraints on the galactic nova rate. | DE K., KASLIWAL M.M., HANKINS M.J., et al. | |
| 2020ATel13967....1R | 247 | T | X | 5 | 2 | ~ |
Carbon Monoxide Emission in Nova Cassiopeiae 2020 ( TCP J00114297+6611190). |
RUSSELL R.W., SITKO M.L., RUDY R.J., et al. | |
| 2020ATel13998....1H | 165 | T | X | 3 | 1 | ~ |
Spectroscopy of Nova Cas 2020 ( TCP J00114297+6611190). |
HAMED G.M., ESENOGLU H.H. and GALEEV A.I. | |
| 2020ATel14004....1S | 412 | T | X | 9 | 1 | ~ |
Spectroscopic observations of Nova Cassiopeiae 2020 = TCP J00114297+6611190 = V1391 Cas. |
SOKOLOVSKY K.V., AYDI E., IZZO L., et al. | |
| 2020ATel14006....1B | 165 | T | X | 3 | 1 | ~ |
Near-infrared spectroscopy of Nova Cas 2020; the persistence of Carbon Monoxide emission. |
BANERJEE D.P.K., SHAHBANDEH M., EVANS A., et al. | |
| 2021JAVSO..49...95S | O | 1 | ~ | The Photometric Period of V1391 Cassiopeiae (Nova Cas 2020). | SCHMIDT R.E. | ||||
| 2020ATel14034....1W | 247 | T | X | 5 | 2 | ~ |
The IR spectral evolution of Nova Sagittarius 2002 #2 and Nova Cassiopeia 2020. |
WOODWARD C.E., BANERJEE D.P.K. and EVANS A. | |
| 2020ATel14267....1M | 288 | T | X | 6 | 1 | ~ |
Nova Cas 2020 (= V1391 Cas) is likely forming dust. |
MUNARI U., BANERJEE D.P.K., CASTELLANI F., et al. | |
| 2020ATel14272....1B | 165 | T | X | 3 | 2 | ~ |
Near-infrared observations confirm Nova Cas 2020 ( V1391 Cas) has formed dust. |
BANERJEE D.P.K., ANUPAMA G.C., MUNARI U., et al. | |
| 2022MNRAS.515.1404H | 639 | X C F | 13 | 16 | ~ | Explaining prolonged fluctuations in light curves of classical novae via modelling. | HILLMAN Y. | ||
| 2022ApJ...937...64K | 17 | D | 1 | 64 | 8 | The Galactic Nova Rate: Estimates from the ASAS-SN and Gaia Surveys. | KAWASH A., CHOMIUK L., STRADER J., et al. | ||
| 2022MNRAS.517.3640S | 17 | D | 1 | 184 | 8 | Comprehensive listing of 156 reliable orbital periods for novae, including 49 new periods. | SCHAEFER B.E. | ||
|
2022MNRAS.517.6150S |
17 | D | 1 | 423 | 10 | Comprehensive catalogue of the overall best distances and properties of 402 galactic novae. | SCHAEFER B.E. | ||
| 2023ApJ...954L..16B | 44 | X | 1 | 21 | ~ | Snowflakes in a Furnace: Formation of CO and Dust in a Recurrent Nova Eruption. | BANERJEE D.P.K., WOODWARD C.E., JOSHI V., et al. | ||
| 2024RNAAS...8...80R | 699 | T A | X C | 14 | 7 | ~ |
CO and C I Emission in the Early Spectrum of the Nova V1391 Cassiopeiae. |
RUDY R.J., RUSSELL R.W., SITKO M.L., et al. | |
| 2024AJ....168..266K | 1254 | T A | D | X C | 27 | 5 | ~ |
Formation of CN and CO Molecules in the Envelope of Nova V1391 Cas During the Near-maximum Phase. |
KAWAKITA H. and LYKE J.E. |
| 2024A&A...692A.264S | 45 | X | 1 | 20 | ~ | Fate and detectability of rare gas hydride ions in nova ejecta A case study with nova templates. | SIL M., DAS A., DAS R., et al. | ||
| 2025ApJ...981..198C | 47 | X | 1 | 50 | ~ | On the Light Curves of Disk and Bulge Novae. | COHEN A., GUETTA D., HILLMAN Y., et al. | ||
| 2025ApJ...982...89S | 93 | X | 2 | 21 | ~ | Hydrodynamic Predictions for the Next Outburst of T Coronae Borealis: It Will Be the Brightest Classical or Recurrent Nova Ever Observed in X-Rays. | STARRFIELD S., BOSE M., WOODWARD C.E., et al. | ||
| 2025MNRAS.538.2339C | 19 | D | 1 | 72 | ~ | Revisiting the classics: on the optical colours of novae as standard crayons. | CRAIG P., AYDI E., CHOMIUK L., et al. | ||
| 2025RNAAS...9..151R | 47 | X | 1 | 5 | ~ | Carbon Monoxide Emission from the 1998 Outburst of the Recurrent Nova V2487 Ophiuchi. | RUDY R.J., LYNCH D.K. and PUETTER R.C. | ||
| 2025RNAAS...9..213S | 75 | A | X | 2 | 7 | ~ | Discovery of 6 New Orbital Periods for Classical Novae. | SCHAEFER B.E. | |
| 2025AJ....170..220B | 19 | D | 1 | 60 | ~ | The Unexplored Dusty Nova LMCN 2009-05a in the Large Magellanic Cloud. | BISHT M.S., RAJ A., WALTER F.M., et al. | ||
| 2025ApJ...993..232S | 19 | D | 1 | 411 | ~ | Comprehensive Listing of 208 Nova White Dwarf Masses as the Primary Determinant of Spectral Class and Light-curve Class. | SCHAEFER B.E. |