activity
20012024
most citedBlack hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

315 citations · 585 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2024

Synthesis and Spectroscopic Characterization of Interstellar Candidate Ethynyl Thiocyanate: HCCSCN

Elena R. Alonso, Aran Insausti, Lucie Kolesniková +7

This work aims to spectroscopically characterize and provide for the first time direct experimental frequencies of the ground vibrational state and two excited states of the simple…

astro-ph.GA2022★ 2 cited

Ionise hard: interstellar PO detection

Víctor M. Rivilla, Juan García de la Concepción, Izaskun Jiménez-Serra +13

We report the first detection of the phosphorus monoxide ion (PO) in the interstellar medium. Our unbiased and very sensitive spectral survey towards the G+0.6930.027 mole…

astro-ph.GA2010★ 21 cited

Herschel observations in the ultracompact HII region Mon R2: Water in dense Photon-dominated regions (PDRs)

A. Fuente, O. Berne, J. Cernicharo +42

Mon R2, at a distance of 830 pc, is the only ultracompact HII region (UC HII) where the photon-dominated region (PDR) between the ionized gas and the molecular cloud can be resolve…

astro-ph.CO2010★ 22 cited

Excitation of the molecular gas in the nuclear region of M82

A. F. Loenen, P. P. van der Werf, R. Güsten +23

We present high resolution HIFI spectroscopy of the nucleus of the archetypical starburst galaxy M82. Six 12CO lines, 2 13CO lines and 4 fine-structure lines are detected. Besides…

astro-ph.GA2010★ 315 cited

Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

P. P. Van der Werf, K. G. Isaak, R. Meijerink +34

We present a full high resolution SPIRE FTS spectrum of the nearby ultraluminous infrared galaxy Mrk231. In total 25 lines are detected, including CO J=5-4 through J=13-12, 7 rotat…

astro-ph2004★ 182 cited

Molecular Gas Chemistry in AGN I. The IRAM Survey of NGC1068

A. Usero, S. Garcia-Burillo, A. Fuente +2

There is observational evidence that nuclear winds and X-rays can heavily influence the physical conditions and chemical abundances of molecular gas in the circumnuclear disks (CND…