High Resolution Mappings of the L=1.3 deg Complex in Molecular Lines : Discovery of a Proto-Superbubble
| dc.creator | Tanaka, Kunihiko | |
| dc.creator | Kamegai, Kazuhisa | |
| dc.creator | Nagai, Makoto | |
| dc.creator | Oka, Tomoharu | |
| dc.date | 2007-01-30 | |
| dc.date.accessioned | 2026-07-07T07:43:45Z | |
| dc.date.available | 2026-07-07T07:43:45Z | |
| dc.description | We report the results of molecular line observations toward the l=1.3 deg complex, ananomalous cloud complex in the central molecular zone of the Galaxy. We have taken high resolution maps of the CO J=1-0, HCN J=1-0, HCO+ J=1-0, SiO J=1-0 and J=2-1 lines. The complex is found to be rich in shells and arcs of dense molecular gas. We have identified 9 expanding shells in HCN maps and compact SiO features associated to the shells. The intensity ratios of HCN/CO, HCO+/CO and CO J=3-2/J=1-0 are coherently enhanced by a factor of a few in gas with an LSR velocity higher than 110 kms^-1. The high-velocity gas has a high density [n_H ~ 10^4.5 cm^-3] and high SiO/13CO intensity ratio indicating that the gas was shocked. The typical HCN/HCO+ intensity ratio is found to be 2.3, being higher by an factor of a few than those in the Galactic disk clouds. The typical kinetic energy and expansion time of the shells are estimated to be 10^(50.9 - 52.5) erg and 10^(4.6 - 5.3) yr, respectively. The kinetic energy could be furnished by multiple supernova and/or hypernova explosions with a rate of 10^(-3 - -4) yr^-1. These estimates suggest that the expanding shells as a whole may be in the early stage of superbubble formation. This proto-superbubble may be originated by a massive cluster formation which took place 10^(6.8 - 7.6) yr ago. | |
| dc.description | 19 pages, 8 figures, to appear in PASJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0701844 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0701844 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/122950 | |
| dc.subject | Astrophysics | |
| dc.title | High Resolution Mappings of the L=1.3 deg Complex in Molecular Lines : Discovery of a Proto-Superbubble | |
| dc.type | text |