other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
Query : 2008MNRAS.386..117J |
2008MNRAS.386..117J - Mon. Not. R. Astron. Soc., 386, 117-137 (2008/May-1)
Spectral imaging of the Sagittarius B2 region in multiple 3-mm molecular lines with the Mopra telescope.
JONES P.A., BURTON M.G., CUNNINGHAM M.R., MENTEN K.M., SCHILKE P., BELLOCHE A., LEURINI S., OTT J. and WALSH A.J.
Abstract (from CDS):
There are significant differences in molecular emission, pointing to both abundance and excitation differences throughout the region. Seven distinct spatial locations are identified for the emitting species, including peaks near the prominent star-forming cores of Sgr B2(N), (M) and (S) that are seen in infrared (IR)-to-radio continuum images. The other features are a `north ridge' and a `north cloud' to the north of the Sgr B2 N-M-S cores, a `south-east peak' and a `west ridge'.
The column density, as evident through C18O, peaks at the Sgr B2(N) and (M) cores, where strong absorption is also evident in otherwise generally bright lines such as HCO+, HCN and HNC. Most molecules trace a ridge line to the west of the Sgr B2 N-M-S cores, wrapping around the cores and extending north-east to the north cloud. This is most clearly evident in the species HC3N, CH3CN, CH3OH and OCS. They are found to be closer in distribution to the cooler dust traced by the submillimetre continuum than either the warmer dust seen in the mid-IR or to the radio continuum. The molecule CN, in contrast, is reasonably uniform over the entire region mapped, aside from strong absorption at the positions of the Sgr B2(N) and (M) cores.
Abstract Copyright: ©2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): ISM: individual: Sagittarius B2 - ISM: kinematics and dynamics - ISM: molecules - radio lines: ISM
Simbad objects: 13
Number of rows : 13 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | GAL 332.80-00.60 | HII | 16 19 47 | -51 04.1 | ~ | 99 | 1 | |||||
2 | NAME Sgr E | Rad | 17 42 38 | -29 48.2 | ~ | 52 | 0 | |||||
3 | NAME Sgr C | MoC | 17 44 36.3 | -29 28 13 | ~ | 354 | 0 | |||||
4 | NAME Sgr A Region | reg | 17 45 12 | -28 48.3 | ~ | 939 | 0 | |||||
5 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 14415 | 0 | |||||
6 | NAME Sgr A* | X | 17 45 40.03599 | -29 00 28.1699 | ~ | 4390 | 3 | |||||
7 | NAME Sgr B1 | MoC | 17 47 02.0 | -28 31 57 | ~ | 164 | 0 | |||||
8 | NAME Sgr B2 (North) | Rad | 17 47 20.2 | -28 22 21 | ~ | 673 | 1 | |||||
9 | NAME Sgr B2 | MoC | 17 47 20.4 | -28 23 07 | ~ | 2266 | 1 | |||||
10 | NAME Sgr B2 (South) | HII | 17 47 20.430 | -28 23 45.06 | ~ | 100 | 0 | |||||
11 | NAME Large Molecule Heimat | MoC | 17 47 20.4943 | -28 22 11.656 | ~ | 123 | 0 | |||||
12 | NAME Sgr B2 Main | Rad | 17 47 20.5 | -28 23 06 | ~ | 407 | 1 | |||||
13 | NAME Sgr D | MoC | 17 48 41.75 | -28 01 45.0 | ~ | 133 | 1 |
To bookmark this query, right click on this link: simbad:objects in 2008MNRAS.386..117J and select 'bookmark this link' or equivalent in the popup menu