most citedFirst detection in space of the high-energy isomer of cyanomethanimine: H2CNCN

41 citations · 77 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025★ 1 cited

High deuteration of methanol in L1544

S. Spezzano, W. Riedel, P. Caselli +7

Isotopic fractionation is a very powerful tool to follow the evolution of material from one stage to the next in the star-formation process. Pre-stellar cores exhibit some of the h…

astro-ph.GA2025★ 3 cited

First Detections of PN, PO, and PO+ toward a Shocked Low-mass Starless Core

Samantha Scibelli, Andrés Megías, Izaskun Jiménez-Serra +6

Phosphorus is a key element that plays an essential role in biological processes important for living organisms on Earth. The origin and connection of phosphorus-bearing molecules…

astro-ph.GA2024★ 1 cited

Discovery of MgS and NaS in the Interstellar Medium and tentative detection of CaO

M. Rey-Montejo, I. Jimenez-Serra, J. Martin-Pintado +12

We report the first detection of the metal-bearing molecules sodium sulfide (NaS) and magnesium sulfide (MgS) and the tentative detection of calcium monoxide (CaO) in the interstel…

astro-ph.GA2024★ 41 cited

First detection in space of the high-energy isomer of cyanomethanimine: H2CNCN

David San Andrés, Víctor M. Rivilla, Laura Colzi +14

We report the first detection in the interstellar medium of -cyanomethanimine (HCNCN), the stable dimer of HCN of highest energy, and the most complex organic molecule ident…

astro-ph.GA2024★ 30 cited

Discovery of thionylimide, HNSO, in space: the first N-, S- and O-bearing interstellar molecule

Miguel Sanz-Novo, Víctor M. Rivilla, Holger S. P. Müller +12

We present the first detection in space of thionylimide (HNSO) toward the Galactic Center molecular cloud G+0.693-0.027, thanks to the superb sensitivity of an ultradeep molecular…

astro-ph.GA2024★ 1 cited

Interstellar detection of O-protonated carbonyl sulfide, HOCS+

Miguel Sanz-Novo, Víctor M. Rivilla, Izaskun Jiménez-Serra +12

We present the first detection in space of O-protonated carbonyl sulfide (\ch{HOCS+}), in the midst of an ultradeep molecular line survey toward the G+0.693-0.027 molecular cloud.…