V* V3662 Oph , the SIMBAD biblio

V* V3662 Oph , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:56:32


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
2017ApJ...851L..30J 437 T K A D S   X         10 15 1
Nova Ophiuchus 2017 as a probe of 13C nucleosynthesis and carbon monoxide formation and destruction in classical novae.
JOSHI V., BANERJEE D.P.K. and SRIVASTAVA M.
2017ATel10975....1L 79 T                   1 2 ~ Spectroscopic Observations of PNV J17184504-2454221 (
Nova Oph 2017) as a Classical Nova in the Iron Curtain Phase.
LUCKAS P.
2017ATel10366....1W 159 T         X         3 2 ~ Spectroscopic classification of
TCP J17394608-2457555 as a Galactic nova.
WILLIAMS S.C. and DARNLEY M.J.
2017ATel10367....1S 119 T         X         2 2 ~ ASAS-SN photometry of the Galactic nova
TCP J17394608-2457555.
STRADER J., CHOMIUK L., BROWN J.S., et al.
2017ATel10369....1J 119 T         X         2 1 ~ First overtone CO detected in emission in Galactic nova
TCP J17394608-2457555.
JOSHI V. and BANERJEE D.P.K.
2017ATel10420....1R 199 T         X         4 4 ~ Optical and near-IR spectroscopy of
nova Oph 2017 (
TCP J17394608-2457555).
RAJ A., PAVANA M., ANUPAMA G.C., et al.
2017ATel10492....1J 199 T         X         4 1 ~ Dust formation in
Nova Oph 2017 (
TCP J17394608-2457555).
JOSHI V., BANERJEE D.P.K. and SRIVASTAVA M.
2017ATel10536....1K 238 T         X         5 1 ~
Nova Oph 2017 (
TCP J17394608-2457555) detected at millimeter wavelengths.
KAMINSKI T. and GEHRZ R.
2020ATel13888....1B 41           X         1 5 ~ Rapid disappearance of Carbon Monoxide emission in Nova 2020Sgr #2. BANERJEE D.P.K., WOODWARD C.E., EVANS A., et al.
2021ApJ...910..120K viz 17       D               1 1667 12 Classical novae masquerading as dwarf novae? Outburst properties of cataclysmic variables with ASAS-SN. KAWASH A., CHOMIUK L., STRADER J., et al.
2021A&A...650A.187S 17       D               1 109 ~ Nucleosynthesis constraints through γ-ray line measurements from classical novae. Hierarchical model for the ejecta of 22Na and 7Be. SIEGERT T., GHOSH S., MATHUR K., et al.
2022A&A...659A.109K 187       D     X         5 129 2 A search for cool molecular gas in GK Persei and other classical novae. KAMINSKI T., MAZUREK H.J., MENTEN K.M., et al.
2022MNRAS.516.1008L 128           X C       2 5 ~ Gamma-ray light curves and spectra of classical novae. LEUNG S.-C. and SIEGERT T.
2022MNRAS.517.6150S viz 17       D               1 423 10 Comprehensive catalogue of the overall best distances and properties of 402 galactic novae. SCHAEFER B.E.
2023MNRAS.523.3555Z 131           X   F     2 86 2 Rapidly evolving Galactic plane outbursts in NEOWISE: revisiting the Galactic nova rate with the first all-sky search in the mid-infrared. ZUCKERMAN L., DE K., EILERS A.-C., et al.
2023ApJ...953..160A 17       D               1 80 ~ Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore. ABBASI R., ACKERMANN M., ADAMS J., et al.
2023ApJ...954L..16B 87           X         2 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.
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.541..980C 205       D       C F     7 50 ~ Revisiting the classics: on the statistics of dust formation in novae. CHONG A., AYDI E., CRAIG P., et al.
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.

goto View the references in ADS