-
Rigel K-band temporal monitoring
Luminous BA-type supergiants are the brightest stars in the visible that can be observed in distant galaxies and are potentially accurate distance indicators. The impact of the... -
Maps and datacubes of NGC 7538 IRS 1
NGC 7538 IRS 1-3 is a high-mass star-forming cluster with several detected dust cores, infrared sources, (ultra)compact HII regions, molecular outflows, and masers. In such a... -
NGC 7129 FIRS 2 interferometric 1-D spectrum
NGC 7129 FIRS 2 (hereafter FIRS 2) is an intermediate-mass (2 to 8M_{sun}) protostar located at a distance of 1250pc. High spatial resolution observations are required to... -
HH 212 CO, CS and 850um ALMA images
We wish to exploit the unmatched combination of high angular resolution, high sensitivity, high-imaging fidelity, and spectral coverage provided by ALMA to shed light on the... -
Intensity maps in the star-forming complex W33
The object W33 is a giant molecular cloud that contains star forming regions at various evolutionary stages from quiescent clumps to developed HII regions. Since its star... -
LOFAR long baselines at 140MHz Calibrators
An efficient means of locating calibrator sources for international LOw Frequency ARray (LOFAR) is developed and used to determine the average density of usable calibrator... -
Starless gas clump IRDC 18310-4 images
We study the fragmentation and collapse properties of the dense gas during the onset of high-mass star formation. We observed the massive (800M_{sun}) starless gas clump IRDC... -
HI data cubes of 4 edge-on spiral galaxies
Edge-on galaxies can offer important insight into galaxy evolution because they are the only systems where the distribution of the different components can be studied both... -
NGC 4418 ALMA mm-wave spectral scan
Extragalactic observations allow the study of molecular chemistry and excitation under physical conditions which may differ greatly from what found in the Milky Way. The... -
TZ For OIFITS files
Independent distance estimates are particularly useful to check the precision of other distance indicators, while accurate and precise masses are necessary to constrain... -
Exoplanetary parameters for 18 bright stars
We present the interferometric angular diameters of 18 bright stars: HD3651 , HD9826, HD19994, HD75732, HD167042, HD170693, HD173416, HD185395, HD190360, HD217014, HD221345,... -
CO, SO and H_2_CO images of AB Aur
Transitional disks are structures of dust and gas around young stars with large inner cavities in which planet formation may occur. Lopsided dust distributions are observed in... -
Class 0 sources continuum subtracted UV-tables
The physical structure of deeply-embedded low-mass protostars (Class 0) on scales of less than 300AU is still poorly constrained. While molecular line observations demonstrate... -
VY CMa ALMA NaCl images
At the end of their lives, most stars lose a significant amount of mass through a stellar wind. The specific physical and chemical circumstances that lead to the onset of the... -
G35.20-0.74N VLA continuum images
Atacama Large Millimeter/submillimeter Array (ALMA) observations of the high-mass star-forming region G35.20-0.74N have revealed the presence of a Keplerian disk in core B... -
delta Cep VEGA/CHARA observing log
The B-W method is used to determine the distance of Cepheids and consists in combining the angular size variations of the star, as derived from infrared surface-brightness... -
eta Car velocity-resolved imaging
The mass loss from massive stars is not understood well. eta Carinae is a unique object for studying the massive stellar wind during the luminous blue variable phase. It is also... -
SAM detection limits of 8 debris disks
The formation of planetary systems is a common, yet complex mechanism. Numerous stars have been identified to possess a debris disk, a proto-planetary disk or a planetary... -
QSO 1308+326 at 15GHz modelfit results
Despite numerous and detailed studies of the jets of Active Galactic Nuclei (AGN) on pc-scales, many questions are still debated. The physical nature of the jet components is... -
NGC1068 interferometric mid-IR measurements
Recent NuSTAR observations revealed a somewhat unexpected increase in the X-ray flux of the nucleus of NGC 1068. We expect the infrared emission of the dusty torus to react on...