activity
20092022
most citedVLT/X-shooter survey of near-infrared diffuse interstellar bands

81 citations · 481 across the 15 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2022★ 9 cited

Near-infrared spectroscopy of embedded protostars in the massive metal-poor star-forming region NGC 346

O. C. Jones, M. Reiter, R. Sanchez-Janssen +4

We present medium-resolution (R 4000) YJ, H \& K band spectroscopy of candidate young stellar objects (YSOs) in NGC~346, the most active star-formation region in the metal-p…

astro-ph.GA2019★ 15 cited

Characterisation of the Planetary Nebula Tc 1 Based on VLT X-Shooter Observations

Isabel Aleman, Marcelo L. Leal-Ferreira, Jan Cami +11

We present a detailed analysis of deep VLT/X-Shooter observations of the planetary nebula Tc 1. We calculate gas temperature, density, extinction, and abundances for several specie…

astro-ph.GA2017

The star-forming complex LMC-N79 as a future rival to 30 Doradus

Bram B. Ochsendorf, Hans Zinnecker, Omnarayani Nayak +5

Within the early Universe, `extreme' star formation may have been the norm rather than the exception. Super Star Clusters (SSCs; 10 M) are thought t…

astro-ph.GA2017★ 51 cited

[CII] emission from L1630 in the Orion B molecular cloud

C. H. M. Pabst, J. R. Goicoechea, D. Teyssier +11

Observations towards L1630 in the Orion B molecular cloud, comprising the iconic Horsehead Nebula, allow us to study the interplay between stellar radiation and a molecular cloud u…

astro-ph.SR2017★ 5 cited

Unidentified emission features in the R Coronae Borealis star V854 Centauri

L. C. Oostrum, B. B. Ochsendorf, L. Kaper +1

During its 2012 decline the R Coronae Borealis star (RCB) V854 Cen was spectroscopically monitored with X-shooter on the ESO Very Large Telescope. The obscured optical and near-inf…

astro-ph.SR2017★ 31 cited

Massive pre-main sequence stars in M17

María Claudia Ramírez-Tannus, Lex Kaper, Alex de Koter +6

The formation process of massive stars is still poorly understood. Massive young stellar objects (mYSOs) are deeply embedded in their parental clouds, they are rare and thus typica…

astro-ph.GA2017★ 57 cited

What sets the massive star formation rates and efficiencies of giant molecular clouds?

Bram B. Ochsendorf, Margaret Meixner, Julia Roman-Duval +2

Galactic star formation scaling relations show increased scatter from kpc to sub-kpc scales. Investigating this scatter may hold important clues to how the star formation process e…

astro-ph.GA2016★ 14 cited

The location, clustering, and propagation of massive star formation in giant molecular clouds

B. B. Ochsendorf, M. Meixner, J. Chastenet +2

Massive stars are key players in the evolution of galaxies, yet their formation pathway remains unclear. In this work, we use data from several galaxy-wide surveys to build an unbi…

astro-ph.GA2016★ 25 cited

Kompaneets Model Fitting of the Orion-Eridanus Superbubble II: Thinking Outside of Barnard's Loop

Andy Pon, Bram B. Ochsendorf, João Alves +3

The Orion star-forming region is the nearest active high-mass star-forming region and has created a large superbubble, the Orion-Eridanus superbubble. Recent work by Ochsendorf et…

astro-ph.SR2016★ 19 cited

XSHOOTER spectroscopy of the enigmatic planetary nebula Lin49 in the Small Magellanic Cloud

Masaaki Otsuka, F. Kemper, M. L. Leal-Ferreira +6

We performed a detailed spectroscopic analysis of the fullerene C60-containing planetary nebula (PN) Lin49 in the Small Magellanic Cloud using XSHOOTER at the ESO VLT and the Spitz…

astro-ph.GA2015★ 65 cited

Nested shells reveal the rejuvenation of the Orion-Eridanus superbubble

B. B. Ochsendorf, A. G. A. Brown, J. Bally +1

The Orion-Eridanus superbubble is the prototypical superbubble due to its proximity and evolutionary state. Here, we provide a synthesis of recent observational data from WISE and…

astro-ph.SR2014★ 22 cited

Depletion of chlorine into HCl ice in a protostellar core

M. Kama, E. Caux, A. Lopez-Sepulcre +9

The freezeout of gas-phase species onto cold dust grains can drastically alter the chemistry and the heating-cooling balance of protostellar material. In contrast to well-known spe…

astro-ph.GA2014★ 14 cited

Kompaneets Model Fitting of the Orion-Eridanus Superbubble

Andy Pon, Doug Johnstone, John Bally +1

Winds and supernovae from OB associations create large cavities in the interstellar medium referred to as superbubbles. The Orion molecular clouds are the nearest high mass star-fo…

astro-ph.GA2014★ 81 cited

VLT/X-shooter survey of near-infrared diffuse interstellar bands

N. L. J. Cox, J. Cami, L. Kaper +5

This paper presents a spectral survey of diffuse interstellar bands (DIBs) in the NIR range, from 0.9 to 2.5 micron. The observations were designed to detect new DIBs, confirm prev…

astro-ph.SR2011★ 24 cited

First firm spectral classification of an early-B pre-main-sequence star: B275 in M17

B. B. Ochsendorf, L. E. Ellerbroek, R. Chini +4

The optical to near-infrared (300 - 2500 nm) spectrum of the candidate massive Young Stellar Object (YSO) B275, embedded in the star forming region M17, has been observed with X-sh…

astro-ph.SR2009★ 49 cited

On the interplay between flaring and shadowing in disks around Herbig Ae/Be stars

B. Acke, M. Min, M. van den Ancker +4

Based on the SED, Herbig stars have been categorized into two observational groups, reflecting their overall disk structure: group I members have disks with a higher degree of flar…