We present a catalogue of ¹²CO(J = 1–0) and ¹³CO(J = 1–0) molecular clouds in the spatio-velocity range of the Carina Flare supershell, GSH287+04-17. The data cover a region of ~66 square degrees and were taken with the NANTEN 4m telescope, at spatial and velocity resolutions of ~2'.06 and 0.1 kms⁻¹. Decomposition of the emission results in the identification of 156 ¹²CO clouds and 60 ¹³CO clouds, for which we provide observational and physical parameters. Previous work suggests the majority of the detected mass forms part of a comoving molecular cloud complex that is physically associated with the expanding shell. The cloud internal velocity dispersions, degree of virialization and size-linewidth relations are found to be consistent with t...
We report the detection of a peculiar molecular cloud, CO 0.02-0.02, lying about 5' Galactic east fr...
We present parsec-scale resolution observations of the atomic and molecular ISM in two Galactic supe...
We present a comparison of molecular clouds (MCs) from a simulation of supernova (SN) driven interst...
The ‘Carina Flare’ supershell, GSH 287+04−17, is a molecular supershell originally discovered in ¹²C...
Empirical thesis.Bibliography: pages 48-54.1. Introduction -- 2. Data -- 3. Identification of young ...
13CO(J = 2–1) and C18O(J = 2–1) observations of the molecular cloud G285.90+4.53 (Cloud 16) in the C...
We present large area, fully-sampled maps of the Carina molecular cloud complex in the CO (J = 4 - 3...
We present an in-depth case study of three molecular clouds associated with the walls of the Galacti...
We carried out an unbiased survey for massive dense cores in the giant molecular cloud associated wi...
We present an in-depth case study of three molecular clouds associated with the walls of the Galacti...
Artículo de publicación ISIContext. The Carina region is an excellent astrophysical laboratory for s...
Context. The Carina nebula hosts a large number of globulettes. An optical study of these tiny molec...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We present parsec-scale resolution observations of the atomic and molecular interstellar medium in t...
We present an analysis of a systematic CO(2–1) survey at 12′′ resolution covering most of the Local ...
We report the detection of a peculiar molecular cloud, CO 0.02-0.02, lying about 5' Galactic east fr...
We present parsec-scale resolution observations of the atomic and molecular ISM in two Galactic supe...
We present a comparison of molecular clouds (MCs) from a simulation of supernova (SN) driven interst...
The ‘Carina Flare’ supershell, GSH 287+04−17, is a molecular supershell originally discovered in ¹²C...
Empirical thesis.Bibliography: pages 48-54.1. Introduction -- 2. Data -- 3. Identification of young ...
13CO(J = 2–1) and C18O(J = 2–1) observations of the molecular cloud G285.90+4.53 (Cloud 16) in the C...
We present large area, fully-sampled maps of the Carina molecular cloud complex in the CO (J = 4 - 3...
We present an in-depth case study of three molecular clouds associated with the walls of the Galacti...
We carried out an unbiased survey for massive dense cores in the giant molecular cloud associated wi...
We present an in-depth case study of three molecular clouds associated with the walls of the Galacti...
Artículo de publicación ISIContext. The Carina region is an excellent astrophysical laboratory for s...
Context. The Carina nebula hosts a large number of globulettes. An optical study of these tiny molec...
Context. New-generation spectroscopic surveys of the Milky Way plane have been revealing the structu...
We present parsec-scale resolution observations of the atomic and molecular interstellar medium in t...
We present an analysis of a systematic CO(2–1) survey at 12′′ resolution covering most of the Local ...
We report the detection of a peculiar molecular cloud, CO 0.02-0.02, lying about 5' Galactic east fr...
We present parsec-scale resolution observations of the atomic and molecular ISM in two Galactic supe...
We present a comparison of molecular clouds (MCs) from a simulation of supernova (SN) driven interst...