Add to ORKGWe combine multi-frequency observations from the millimeter to near infrared wavelengths that demonstrate the spatial distributions of H2, CO, and NH3 emission, which are all manifestations of various shocks driven by outflows of deeply embedded source(s) in NGC 6334I. In addition to the well-known northeast-southwest outflow we detect at least one more outflow in the region by combining observations from APEX, ATCA, SMA, Spitzer and VLT/ISAAC. Potential driving sources will be discussed. NGC 6334I exhibits several signs of active star formation and will be a major target for future observatories such as Herschel and ALMA
International audienceAims: We present observations of twelve rotational transitions of H_216O, H_21...
Aims. The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal...
International audienceContext. In contrast to the more extensively studied dense star-forming cores,...
NGC 6334 (1=351°.1, b=0°.7, distance = 1.7 kpc) is a region where multiple star formation has occurr...
The region centered in the NGC 6334 I(N) radio continuum source was surveyed in an extension of 6 ar...
Aims.The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal ...
Molecular line observations of NH3 (J ; K) ¼ (1; 1) and (2, 2) and CH3OH at 24.93 GHz taken with the...
We present results of high-sensitivity, high-resolution, multifrequency VLA observations toward the ...
Aims:We investigate the dense gas, the outflows, and the continuum emission from the massive twin co...
We present a high-resolution, multi-wavelength study of the massive protostellar cluster NGC 6334 I(...
Infrared photometry and maps from 2 to 100 microns are presented for three of the principal far infr...
We present a high-resolution, multi-wavelength study of the massive protostellar cluster NGC 6334 I(...
Aims. The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal...
Aims. We aim at deriving the molecular abundances and temperatures of the hot molecular cores in the...
International audienceAims: We present observations of twelve rotational transitions of H_216O, H_21...
Aims. The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal...
International audienceContext. In contrast to the more extensively studied dense star-forming cores,...
NGC 6334 (1=351°.1, b=0°.7, distance = 1.7 kpc) is a region where multiple star formation has occurr...
The region centered in the NGC 6334 I(N) radio continuum source was surveyed in an extension of 6 ar...
Aims.The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal ...
Molecular line observations of NH3 (J ; K) ¼ (1; 1) and (2, 2) and CH3OH at 24.93 GHz taken with the...
We present results of high-sensitivity, high-resolution, multifrequency VLA observations toward the ...
Aims:We investigate the dense gas, the outflows, and the continuum emission from the massive twin co...
We present a high-resolution, multi-wavelength study of the massive protostellar cluster NGC 6334 I(...
Infrared photometry and maps from 2 to 100 microns are presented for three of the principal far infr...
We present a high-resolution, multi-wavelength study of the massive protostellar cluster NGC 6334 I(...
Aims. The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal...
Aims. We aim at deriving the molecular abundances and temperatures of the hot molecular cores in the...
International audienceAims: We present observations of twelve rotational transitions of H_216O, H_21...
Aims. The massive twin cores NGC 6334I and I(N) are in different evolutionary stages and hence ideal...
International audienceContext. In contrast to the more extensively studied dense star-forming cores,...