AT 2020hat , the SIMBAD biblio

AT 2020hat , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:48:01


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Title First 3 Authors
2020ATel13642....1R 128 T         X         2 6 ~ Radio observations of SN 2020fqv, SN 2020fsb and
AT 2020hat.
RYDER S.D., KUNDU E., FILIPOVIC M.D., et al.
2020ATel13644....1R 128 T         X         2 3 ~ Spectroscopic classification of
AT2020hat in NGC 5068 by NUTS2 (NOT Un-biased Transient Survey-2).
REGUITTI A., PASTORELLO A., ELIAS-ROSA N., et al.
2021A&A...646A.119P viz 262         O X C       5 16 19 Forbidden hugs in pandemic times. I. Luminous red nova AT 2019zhd, a new merger in M 31. PASTORELLO A., FRASER M., VALERIN G., et al.
2021A&A...647A..93P viz 3439 T K A D S   X C       77 25 18 Forbidden hugs in pandemic times. II. The luminous red nova variety:
AT 2020hat and AT 2020kog.
PASTORELLO A., VALERIN G., FRASER M., et al.
2021A&A...653A.134B viz 193       D     X         5 33 33 The luminous red nova AT 2018bwo in NGC 45 and its binary yellow supergiant progenitor. BLAGORODNOVA N., KLENCKI J., PEJCHA O., et al.
2021MNRAS.507..385H 44           X         1 6 2 Simulating a stellar contact binary merger - I. Stellar models. HATFULL R.W.M., IVANOVA N. and LOMBARDI J.C.
2022MNRAS.514.1188B 242       D     X C       5 45 14 Nothing to see here: failed supernovae are faint or rare. BYRNE R.A. and FRASER M.
2022ApJ...937...96M 45           X         1 14 4 Dusty, Self-obscured Transients from Stellar Coalescence. MacLEOD M., DE K. and LOEB A.
2022ApJ...938....5M 64       D     X         2 15 20 Light-curve Model for Luminous Red Novae and Inferences about the Ejecta of Stellar Mergers. MATSUMOTO T. and METZGER B.D.
2023A&A...671A.158P viz 532       D   O X C       11 41 5 Forbidden hugs in pandemic times IV. Panchromatic evolution of three luminous red novae. PASTORELLO A., VALERIN G., FRASER M., et al.
2023ApJ...948..137K 392       D     X         9 68 5 Volumetric Rates of Luminous Red Novae and Intermediate-luminosity Red Transients with the Zwicky Transient Facility. KARAMBELKAR V.R., KASLIWAL M.M., BLAGORODNOVA N., et al.

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