13CO and C18O J = 2–1 mapping of the environment of the Class 0 ...

We attempt to achieve a better understanding of the gas distribution and velocity field around the deeply embedded Class 0 protostar SMM 3 in the Orion B9 star ...

[1208.0673] 13CO and C18O J=2-1 mapping of the environment of ...

We attempt to achieve a better understanding of the gas distribution and velocity field around the deeply embedded Class 0 protostar SMM 3 in the Orion B9 star ...

13 CO and C 18 OJ = 2-1 mapping of the environment ... - NASA ADS

... Class 0 protostar SMM 3 in the Orion B9 star-forming region. Methods: Using the APEX 12-m telescope, we mapped the line emission from the J = 2-1 rotational ...

13CO and C18OJ = 2–1 mapping of the environment of the Class 0 ...

... Class 0 protostar SMM 3 in the Orion B9 star-forming region. Using the APEX 12-m telescope, we mapped the line emission from the J=2-1 rotational transition ...

A 13CO AND C18O SURVEY OF THE MOLECULAR GAS AROUND ...

their environment, we present fully sampled maps in the J = 1–0 lines of 13CO and C18O and the J = 2–1 line of C18O for a selected group of 30 young stellar ...

13CO and C18O J=2-1 mapping of the environment of the Class 0 ...

13CO and C18O J=2-1 mapping of the environment of the Class 0 protostellar core SMM 3 in Orion B9 · : · › · › · › ...

A 13CO and C18O Survey of the Molecular Gas Around Young ...

... mapped with 47'' resolution simultaneously in the two J = 1–0 lines at the Five College Radio Astronomy Observatory. Seventeen sources were mapped over ...

13CO and C18OJ = 2–1 mapping of the environment of the Class 0 ...

13CO and C18OJ = 2–1 mapping of the environment of the Class 0 protostellar core SMM 3 in Orion B9 · List of references · Publications that cite this publication.

Velocity-integrated intensity map of 13 CO J = 2 − 1 emission. The...

Spectra of the J=1-0 transitions from CO, 13CO, and C18O at the centers of the 250 cores were extracted from previous mapping observations to construct a multi- ...

The young cluster in the CB34 globule: the clumps and the outflows

Figure 2. Contour maps of the J = 2–1 13CO (upper panel), J = 1–0. C18O (middle panel), and J = 3–2 CS (lower panel) integrated emission towards CB34 ...

C18O, 13CO, and 12CO abundances and excitation temperatures

21 H cm−2 mag−1. 2.3. Field of view. We aimed to jointly analyze the J = 1−0 and J = 2−1 lines of the CO isotopologues. We thus restricted the field of ...

CO isotopologues in the Perseus Molecular Cloud Complex

data to measure dust extinction; 2) use dust temperatures derived from re-processed. IRAS data; and 3) make use of the 12CO and 13CO (1-0) transition maps ...

A submillimetre survey of the kinematics of the Perseus molecular ...

We selected the four largest clusters of continuum cores – NGC. 1333, IC348, L1448 and L1455 – to map in the 12CO, 13CO and. C18O J = 3 → 2 lines (see Fig. 1; ...

1 and 12 CO J = 3 − 2 emission lines at the... - ResearchGate

Spectra of the J=1-0 transitions from CO, 13CO, and C18O at the centers of the 250 cores were extracted from previous mapping observations to construct a multi- ...

Mapping protostellar outflow shocks in the Serpens South dense cloud

Class 0 to II produce bipolar jets and outflows. Jets are very collimated stream moving at supersonic speed (∼100 km.s−1. (Bjerkeli et al., 2013)) and ...

[PDF] A mapping study of L1174 with 13CO J=2-1 and 12CO J=3-2 ...

J. Yuan, Y. Wu, +4 authors. U. Koln · Published 7 November 2012 · Physics, Environmental Science · Monthly Notices of the Royal Astronomical Society.

TIMES. I. A Systematic Observation in Multiple Molecular Lines ...

J = 1−0 lines of 13CO, C18O, HCN, HCO. +. , and N2H. + and the J = 2−1 line of CS. The fully sampled maps with uniform noise levels are used to create moment ...

IRAM-30m large scale survey of 12CO(2-1) and 13CO(2-1) emission ...

Using 12CO, 13CO and C18O observations,. Castets et al. (1990) provided a column density and an H2 density map of the ISF with an angular resolution of the ...

Symmetry properties and widths of the filamentary structures in the ...

(c) H2 column density map derived from C18O J=1–0 emission. The color scales in the three panels are identical and range from 1.5 × 1020 cm−2 to 1.35 × 1023 cm− ...

PROPOSAL FOR THE 30M TELESCOPE - IRAM

The present proposal aims at improving last year's data on the C18O(1-0) and (2-1) lines in the Cepheus star-forming region to extend the maps ...