TY  - GEN 
AU  - Cai, Y.-Z.
AU  - Pastorello, A.
AU  - Fraser, M.
AU  - Prentice, S.J.
AU  - Reynolds, T. M.
AU  - Cappellaro, E.
AU  - Benetti, S.
AU  - Morales Garoffolo, Antonia Isabel
AU  - Reguitti, A.
AU  - Elias-Rosa, N.
AU  - Brennan, S.
AU  - Callis, E.
AU  - Cannizzaro, G.
AU  - Fiore, A.
AU  - Gromadzki, M.
AU  - Galindo-Guil, F. J.
AU  - Gall, C.
AU  - Heikkilä, T.
AU  - Mason, E.
AU  - Moran, S.
AU  - Onori, F.
AU  - Sagués Carracedo, A.
AU  - Valerin, G.
A4  - Física Aplicada
PY  - 2019
SN  - 0004-6361
SN  - 1432-0746
UR  - http://hdl.handle.net/10498/22283
AB  - Context. The absolute magnitudes of luminous red novae (LRNe) are intermediate between those of novae and supernovae (SNe), and show a relatively homogeneous spectro-photometric evolution. Although they were thought to derive from core instabilities...
LA  - eng
PB  - EDP SCIENCES S A
KW  - binaries: close
KW  - stars: winds, outflows
KW  - stars: massive
KW  - supernovae: individual: AT 2018hso
KW  - supernovae: individual: AT 2017jfs
KW  - supernovae: individual: NGC4490-2011OT1
TI  - The transitional gap transient AT 2018hso: new insights into the luminous red nova phenomenon
DO  - 10.1051/0004-6361/201936749
ER  -