activity
20052013
most citedA deep look into the cores of young clusters I. sigma-Orionis

42 citations · 201 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2013★ 13 cited

CEN34 -- High-Mass YSO in M17 or Background Post-AGB Star?

Zhiwei Chen, Dieter Nuernberger, Rolf Chini +3

We investigate the proposed high-mass young stellar object (YSO) candidate CEN34, thought to be associated with the star forming region M17. Its optical to near-infrared (550-2500…

astro-ph.SR2009★ 19 cited

A deep look into the core of young clusters. II. lambda-Orionis

H. Bouy, N. Huelamo, D. Barrado y Navascues +14

Over the past years, the lambda-Orionis cluster has been a prime location for the study of young very low mass stars, substellar and isolated planetary mass objects and the determi…

astro-ph2008★ 42 cited

Optical and infrared flares from a transient Galactic soft gamma-ray repeater

A. J. Castro-Tirado, A. de Ugarte Postigo, J. Gorosabel +33

Soft gamma-ray repeaters (SGRs) are a rare type of gamma-ray transient sources that are ocasionally detected as bursts in the high-energy sky. They are thought to be produced by ma…

astro-ph2008★ 42 cited

A deep look into the cores of young clusters I. sigma-Orionis

H. Bouy, N. Huelamo, E. L. Martin +9

Nearby young clusters are privileged places to study the star formation history. Over the last decade, the sigma-Orionis cluster has been a prime location for the study of young ve…

astro-ph2007

VLTI/MIDI Observations of the Massive Protostellar Candidate NGC 3603 IRS 9A

Stefan Vehoff, Dieter E. A. Nuernberger, Christian A. Hummel +1

We used MIDI, the mid-infrared interferometric instrument of the VLTI, to observe the massive protostellar candidate IRS 9A, located at a distance of about 7 kpc at the periphery o…

astro-ph2007★ 38 cited

On the infant weight loss of low- to intermediate-mass star clusters

C. Weidner, P. Kroupa, D. E. A. Nuernberger +1

Star clusters are born in a highly compact configuration, typically with radii of less than about 1 pc roughly independently of mass. Since the star-formation efficiency is less th…