activity
20062021
most citedOrganic Molecules in the Galactic Center. Hot Core Chemistry without Hot Cores

119 citations · 175 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2021

CON-quest: Searching for the most obscured galaxy nuclei

N. Falstad, S. Aalto, S. König +28

Some luminous and ultraluminous infrared galaxies (LIRGs and ULIRGs) host extremely compact and dusty nuclei. The intense infrared radiation arising from warm dust in these sources…

astro-ph.GA20205 cited

On the effects of UV photons/X-rays on the chemistry of the Sgr B2 cloud

J. Armijos-Abendaño, J. Martín-Pintado, E. López +7

The lines of HOC, HCO and CO are considered good tracers of photon-dominated regions (PDRs) and X-ray dominated regions. We study these tracers towards regions of the Sgr B…

astro-ph.GA2018

Abundant Z-cyanomethanimine in the interstellar medium: paving the way to the synthesis of adenine

V. M. Rivilla, J. Martín-Pintado, I. Jiménez-Serra +6

We report the first detection in the interstellar medium of the Z-isomer of cyanomethanimine (HNCHCN), an HCN dimer proposed as precursor of adenine. We identified six transitions…

astro-ph.GA2018

Molecular gas in the northern nucleus of Mrk273: Physical and chemical properties of the disk and its outflow

R. Aladro, S. König, S. Aalto +12

Aiming to characterise the properties of the molecular gas in the ultraluminous infrared galaxy Mrk273 and its outflow, we used the NOEMA interferometer to image the dense gas mole…

astro-ph.GA2018

Study of diffuse HII regions potentially forming part of the gas streams around Sgr A*

J. Armijos-Abendaño, E. López, J. Martín-Pintado +8

We present a study of diffuse extended ionised gas toward three clouds located in the Galactic Centre (GC). One line of sight (LOS) is toward the 20 km s cloud (LOS0.11)…

astro-ph.GA201727 cited

Detection of CH+, SH+, and their 13C- and 34S- isotopologues toward PKS1830-211

S. Muller, H. S. P. M"uller, J. H. Black +13

The z=0.89 molecular absorber toward PKS1830-211 provides us with the opportunity to probe the chemical and physical properties of the interstellar medium in the disk of a galaxy a…