activity
20082022
most citedA line confusion limited millimeter survey of Orion KL (I): sulfur carbon chains

174 citations · 2.1k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.GA2022★ 88 cited

Discovery of fulvenallene in TMC-1 with the QUIJOTE line survey

José Cernicharo, Raúl Fuentetaja, Marcelino Agúndez +6

We report the detection of fulvenallene (-CHCCH) in the direction of TMC-1 with the QUIJOTE line survey. Thirty rotational transitions with =0,1,2,3 and =9-1…

astro-ph.GA2022★ 26 cited

Discovery of five cyano derivatives of propene with the QUIJOTE line survey

José Cernicharo, Raúl Fuentetaja, Carlos Cabezas +5

We report the discovery of five cyano derivatives of propene towards TMC-1 with the QUIJOTE line survey: and -crotononitrile (-CHCHCHCN, -CHCHCHCN), meth…

astro-ph.GA2022★ 21 cited

Discovery of the cyclic C5H radical in TMC-1

Carlos Cabezas, Marcelino Agundez, Raul Fuentetaja +6

Cyclic C5H (c-C5H), the radical formed by substituting an ethynyl group CCH for the hydrogen atom in the c-C3H radical, has been detected for the first time in the space. The c-C5H…

astro-ph.GA2021★ 20 cited

Discovery of interstellar 3-cyano propargyl radical, CH2CCCN

Carlos Cabezas, Marcelino Agundez, Nuria Marcelino +4

We report the first detection in interstellar space of the 3-cyano propargyl radical (CH2C3N). This species was observed in the cold dark cloud TMC-1 using the Yebes 40m telescope.…

astro-ph.GA2021★ 47 cited

A study of C4H3N isomers in TMC-1: line by line detection of HCCCH2CN

N. Marcelino, B. Tercero, M. Agundez +1

We present Yebes 40m telescope observations of the three most stable C4H3N isomers towards the cyanopolyyne peak of TMC-1. We have detected 13 transitions from CH3C3N (A and E spec…

astro-ph.GA2020★ 59 cited

Tentative detection of HC5NH+ in TMC-1

N. Marcelino, M. Agundez, B. Tercero +5

Using the Yebes 40m radio telescope, we report the detection of a series of seven lines harmonically related with a rotational constant B0=1295.81581 +/- 0.00026 MHz and a distorti…