activity
20172023
most citedPENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

76 citations · 183 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2023

Snowflakes in a furnace: formation of CO and dust in a recurrent nova eruption

D. P. K. Banerjee, C. E. Woodward, V. Joshi +7

We report the detection of carbon monoxide (CO) and dust, formed under hostile conditions, in recurrent nova V745 Sco about 8.7 days after its 2014 outburst. The formation of molec…

astro-ph.SR2023★ 7 cited

Multiband Photometry Evolution in the First Weeks of SN 2023ixf, a possible II-L Subtype Supernova

Bianciardi G., Ciccarelli A. M., Conzo G. +8

Multiband photometric observations and their evaluation to instrumental magnitudes were performed using standard Johnson-Cousins filters (B, V, Rc) as well r and g Sloan filters, a…

astro-ph.HE2022★ 12 cited

Taking a break: paused accretion in the symbiotic binary RT Cru

A. Pujol, G. J. M. Luna, K. Mukai +10

Symbiotic binaries sometimes hide their symbiotic nature for significant periods of time. There is mounting observational evidence that in those symbiotics that are powered solely…

astro-ph.HE2022★ 2 cited

Persistent nuclear burning in Nova Sgr 2016 N.4 (= V5856 Sgr = ASASSN-16ma) six years past its outburst

U. Munari, N. Masetti, F. M. Walter +4

We report on the fast Nova Sgr 2016 N.4 being surprisingly trapped in a long-lasting and bright plateau (Delta I >= 10 mag above quiescence) six years past the nova eruption. Very…

astro-ph.SR2022★ 3 cited

The recurrent nova V3890~Sgr: a near-infrared and optical study of the red giant component and its environment

B. Kaminsky, A. Evans, Ya. V. Pavlenko +8

We present an analysis of the red giant component of the recurrent nova V3890 Sgr, using data obtained before and after its 2019 eruption. Its effective temperature is $T_{\rm eff}…

astro-ph.SR2022★ 37 cited

The ODYSSEUS Survey. Motivation and First Results: Accretion, Ejection, and Disk Irradiation of CVSO 109

C. C. Espaillat, G. J. Herczeg, T. Thanathibodee +59

The Hubble UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Director's Discretionary Program of low-mass pre-main-sequence stars, coupled with forthcoming data fro…

astro-ph.SR2021★ 1 cited

PENELLOPE II. CVSO 104: a pre-main sequence close binary with an optical companion in Ori OB1

A. Frasca, H. M. J. Boffin, C. F. Manara +14

We present results of our study of the close pre-main sequence spectroscopic binary CVSO 104 in Ori OB1, based on data obtained within the PENELLOPE legacy program. We derive, for…

astro-ph.SR2021

The 2019 outburst of the 2005 classical nova V1047 Cen: a record breaking dwarf nova outburst or a new phenomenon?

E. Aydi, K. V. Sokolovsky, J. S. Bright +28

We present a detailed study of the 2019 outburst of the cataclysmic variable V1047~Cen, which hosted a classical nova eruption in 2005. The peculiar outburst occurred 14 years afte…

astro-ph.SR2021★ 76 cited

PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and -Orionis

C. F. Manara, A. Frasca, L. Venuti +69

The evolution of young stars and disks is driven by the interplay of several processes, notably accretion and ejection of material. Critical to correctly describe the conditions of…

astro-ph.HE2020★ 25 cited

The 2019 eruption of recurrent nova V3890 Sgr: observations by Swift, NICER and SMARTS

K. L. Page, N. P. M. Kuin, A. P. Beardmore +6

V3890 Sgr is a recurrent nova which has been seen in outburst three times so far, with the most recent eruption occurring on 2019 August 27 UT. This latest outburst was followed in…

astro-ph.HE2017★ 20 cited

The Peculiar Multi-Wavelength Evolution Of V1535 Sco

J. D. Linford, L. Chomiuk, T. Nelson +8

We present multi-wavelength observations of the unusual nova V1535 Sco throughout its outburst in 2015. Early radio observations were consistent with synchrotron emission, and earl…