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N2H+(1-0) maps of Ophiuchus main cloud
The earliest phases of clustered star formation and the origin of the stellar initial mass function (IMF) are currently much debated. In order to constrain the origin of the... -
12CO outflows towards submm cores in Perseus
We present a search for outflows towards 51 submillimetre cores in Perseus. With consistently derived outflow properties from a large homogeneous dataset within one molecular... -
Velocities of OMC-1 flows
Observations are reported of H_2_ IR emission in the S(1) v=1-0 line at 2.121{mu}m in the Orion Molecular Cloud, OMC1, using the GriF instrument on the Canada-France-Hawaii... -
Catalogue of high velocity molecular outflows (Update)
This catalog is an up-date of Wu et al., 1996, Cat. . Cone search capability for table J/A+A/426/503/table1a (CO outflows, and their basic parameters) -
H_2_ flows in rho Ophiuchi A
We present an unbiased search for molecular hydrogen emission in the L1688 cloud within the rho Ophiuchi molecular cloud complex. Our near-infrared survey covers a connected... -
C_5_H_2_ Radiatively allowed transitions
Laboratory detection of four isomers of C_5_H_2_ molecule have been reported by Travers et al. (1997ApJ...483L.135T), McCarthy et al. (1997, Science, 275, 518), and Gottlieb et... -
Interstellar bands and H2, CH, CO column densities
Mutual relations between column densities of H_2_, CH and CO molecules as well as between the latter and strengths of the major 5780 and 5797 diffuse bands are presented and... -
Ortho:para-H2 ratio in C and J shocks
Tables 2a-f and 4a-f contain an extensive set of parameters derived from our grid of C-type (tables 2a-f) and J-type (tables 4a-f) planar stationary shock models. Models of... -
NaI in Local Bubble
We present preliminary results form a long-term program of mapping the neutral absorption characteristics of the local interstellar medium, taking advantage of Hipparcos stellar... -
330-360GHz spectral lines of G 34.3+0.15. II.
Tables 5 and 6 present calculated column densities (in units of molecules per cm^2^) of various species in the ultracompact core (UCC), the compact core (CC) and the halo,... -
Laboratory spectroscopy of isobutene
Isobutene ((CH_3_)2_C=CH_2) is one of the four isomers of butene (C_4_H_8_). After the detection of propene (CH_3_CH=CH_2_) toward TMC-1, and also in the warmer environment of... -
Spectroscopy of 299 galaxies from NewHa survey
Using a sample of 299 H{alpha}-selected galaxies at z~~0.8, we study the relationship between galaxy stellar mass, gas-phase metallicity, and star formation rate (SFR), and... -
NIKA view of two star-forming IRDCs
The thermal emission of dust grains is a powerful tool for probing cold, dense regions of molecular gas in the interstellar medium, and so constraining dust properties is key to... -
Data cubes of observed species toward Messier 8
Messier 8 (M8) is one of the brightest HII regions in the sky. We collected an extensive dataset comprising multiple submillimeter spectral lines from neutral and ionized carbon... -
Galactic cold cores. VI. List of Herschel fields
The Galactic Cold Cores project has carried out Herschel photometric observations of 116 fields where the Planck survey has found signs of cold dust emission. The fields contain... -
Galactic Cold Cores. IV. Cold sub-mm sources
For the project Galactic cold cores, Herschel photometric observations were carried out as a follow-up of cold regions of interstellar clouds previously identified with the... -
Catalog of dense cores in Aquila from Herschel
We present and discuss the results of the Herschel Gould Belt survey (HGBS) observations in an ~11deg^2^ area of the Aquila molecular cloud complex at d~260pc, imaged with the...
