activity
20122018
most citedHerschel far-infrared observations of the Carina Nebula complex I: Introduction and global cloud structure

69 citations · 365 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2018★ 64 cited

Surround & Squash: The Interstellar Medium around Scorpius Centaurus OB2

Martin G. H. Krause, Andreas Burkert, Roland Diehl +7

We exploited observational constraints on stars, gas and nucleosynthesis ashes for the closest region of recent massive-star formation, Scorpius-Centaurus OB2, and combined them wi…

astro-ph.GA2017★ 15 cited

Squeezed between shells? On the origin of the Lupus I molecular cloud. - II. APEX CO and GASS HI observations

B. Gaczkowski, V. Roccatagliata, S. Flaischlen +7

[Abridged] The Lupus I cloud is found between the Upper-Scorpius and the Upper-Centaurus-Lupus sub-groups, where the expanding USco HI shell appears to interact with a bubble curre…

astro-ph.SR2017★ 11 cited

Chandra X-ray observation of the young stellar cluster NGC 3293 in the Carina Nebula Complex

T. Preibisch, S. Flaischlen, B. Gaczkowski +2

We characterize the stellar population of the poorly explored young stellar cluster NGC 3293 at the northwestern periphery of the Carina Nebula Complex, in order to evaluate the cl…

astro-ph.SR2015★ 20 cited

Squeezed between shells? On the origin of the Lupus I molecular cloud. APEX/LABOCA, Herschel, and Planck observations

Benjamin Gaczkowski, Thomas Preibisch, Thomas Stanke +7

The Lupus I cloud is found between the Upper-Scorpius (USco) and the Upper-Centaurus-Lupus (UCL) sub-groups of the Sco-Cen OB-association, where the expanding USco H I shell appear…

astro-ph.GA2015★ 18 cited

A network of filaments detected by Herschel in the Serpens Core: A laboratory to test simulations of low-mass star formation

V. Roccatagliata, J. E. Dale, T. Ratzka +6

Filaments represent a key structure during the early stages of the star formation process. Simulations show filamentary structure commonly formed before and during the formation of…

astro-ph.SR2013★ 61 cited

Herschel far-infrared observations of the Carina Nebula Complex. - III: Detailed cloud structure and feedback effects

Veronica Roccatagliata, Thomas Preibisch, Thorsten Ratzka +1

The Carina Nebula complex (CNC) represents one of the most massive star-forming regions in our Galaxy and shows strong feedback from the high massive stars. We use our Herschel FIR…

astro-ph.GA2013★ 38 cited

Discovering young stars in the Gum 31 region with infrared observations

Henrike Ohlendorf, Thomas Preibisch, Benjamin Gaczkowski +4

Context. The Gum 31 bubble containing the stellar cluster NGC 3324 is a poorly-studied young region close to the Carina Nebula. Aims. We are aiming to characterise the young stella…

astro-ph.GA2012★ 44 cited

Herschel far-infrared observations of the Carina Nebula complex II: The embedded young stellar and protostellar population

Benjamin Gaczkowski, Thomas Preibisch, Thorsten Ratzka +3

The Carina Nebula represents one of the largest and most active star forming regions known in our Galaxy with numerous very massive stars.Our recently obtained Herschel PACS & SPIR…

astro-ph.GA2012★ 69 cited

Herschel far-infrared observations of the Carina Nebula complex I: Introduction and global cloud structure

Thomas Preibisch, Veronica Roccatagliata, Benjamin Gaczkowski +1

The Carina Nebula represents one of the most massive galactic star forming regions and displays a high level of massive star feedback. We used SPIRE and PACS onboard of Herschel to…

astro-ph.GA2012★ 25 cited

Jet-driving protostars identified from infrared observations of the Carina Nebula complex

Henrike Ohlendorf, Thomas Preibisch, Benjamin Gaczkowski +3

Aims: Jets are excellent signposts for very young embedded protostars, so we want to identify jet-driving protostars as a tracer of the currently forming generation of stars in the…