activity
20072020
most citedAPEX-CHAMP+ high-J CO observations of low-mass young stellar objects: IV. Mechanical and radiative feedback

107 citations · 433 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2020★ 7 cited

Studying the effects and cause of the massive star formation in Messier 8 East

M. Tiwari, K. M. Menten, F. Wyrowski +4

Messier 8 (M8), one of the brightest HII regions in our Galaxy, is associated with two prominent massive star-forming regions: M8-Main, the particularly bright part of the large sc…

astro-ph.GA2020★ 45 cited

[CII] 158 μm self-absorption and optical depth effects

C. Guevara, J. Stutzki, V. Ossenkopf-Okada +7

Context. The [CII] 158 μm far-infrared (FIR) fine-structure line is one of the most important cooling lines of the star-forming interstellar medium (ISM). High spectral resolution…

astro-ph.GA2019★ 9 cited

Observational study of hydrocarbons in the bright photodissociation region of Messier 8

M. Tiwari, K. M. Menten, F. Wyrowski +3

Hydrocarbons are ubiquitous in the interstellar medium, but their formation is still not well understood, depending on the physical environment they are found in. M8 is host to one…

astro-ph.GA2018★ 24 cited

A thorough view of the nuclear region of NGC 253 - Combined Herschel, SOFIA and APEX dataset

J. P. Pérez-Beaupuits, R. Güsten, A. Harris +5

We present a large set of spectral lines detected in the central region of the starburst galaxy NGC 253. Observations were obtained with the three instruments SPIRE, PACS and…

astro-ph.GA2018★ 9 cited

Unveiling the remarkable photodissociation region of M8

M. Tiwari, K. M. Menten, F. Wyrowski +5

Messier 8 is one of the brightest HII regions in the sky. Using SOFIA, APEX 12 m and IRAM 30 m telescopes, we have performed a comprehensive imaging survey of the emission from the…

astro-ph.GA2015★ 13 cited

Disentangling the excitation conditions of the dense gas in M17 SW

J. P. Pérez-Beaupuits, R. Güsten, M. Spaans +7

We probe the chemical and energetic conditions in dense gas created by radiative feedback through observations of multiple CO, HCN and HCO transitions toward the dense core of…

astro-ph.SR2015★ 19 cited

Outflow forces in intermediate mass star formation

T. A. van Kempen, M. R. Hogerheijde, E. F. van Dishoeck +22

Intermediate mass protostarsprovide a bridge between theories of low- and high-mass star formation. Emerging molecular outflows can be used to determine the influence of fragmentat…

astro-ph.SR2015★ 107 cited

APEX-CHAMP+ high-J CO observations of low-mass young stellar objects: IV. Mechanical and radiative feedback

Umut A. Yıldız, Lars E. Kristensen, Ewine F. van Dishoeck +14

During the embedded stage of star formation, bipolar molecular outflows and UV radiation from the protostar are important feedback processes. Our aim is to quantify the feedback, m…

astro-ph.CO2013★ 45 cited

The nature of the ISM in galaxies during the star-formation activity peak of the Universe

G. Popping, J. P. Pérez-Beaupuits, M. Spaans +2

We combine a semi-analytic model of galaxy formation, tracking atomic and molecular phases of cold gas, with a three-dimensional radiative-transfer and line tracing code to study t…

astro-ph.CO2011★ 23 cited

The deeply obscured AGN of NGC4945 I. Spitzer-IRS maps of [Ne V], [Ne II], H2 0-0 S(1), S(2), and other tracers

J. P. Pérez-Beaupuits, H. W. W. Spoon, M. Spaans +1

The nearly edge-on galaxy NGC4945 is one of the closest galaxies where an AGN and starburst coexist, and is one of the brightest sources at 100 keV. Near and mid-infrared spectrosc…

astro-ph.CO2011★ 43 cited

A Survey of HC3N in Extragalactic Sources - Is HC3N a Tracer of Activity in ULIRGs?

J. E. Lindberg, S. Aalto, F. Costagliola +3

Context. HC3N is a molecule that is mainly associated with Galactic star-forming regions, but it has also been detected in extragalactic environments. Aims. To present the first ex…

astro-ph.GA2009★ 23 cited

CHAMP+ observations of warm gas in M17 SW

J. P. Pérez-Beaupuits, M. Spaans, M. R. Hogerheijde +3

Since the main cooling lines of the gas phase are important tracers of the interstellar medium in Galactic and extragalactic sources, proper and detailed understanding of their emi…

astro-ph2007★ 66 cited

HNC, HCN and CN in Seyfert galaxies

J. P. Pérez-Beaupuits, S. Aalto, H. Gerebro

Bright HNC 1--0 emission has been found towards several Seyfert galaxies. This is unexpected since traditionally HNC is a tracer of cold (10 K) gas, and the molecular gas of lumino…