1995A&A...302L..25M


Query : 1995A&A...302L..25M

1995A&A...302L..25M - Astronomy and Astrophysics, volume 302L25-28 (1995/10-3)

Molecular and atomic fractionation effects in the NGC 1977 molecular cloud.

MINCHIN N.R. and WHITE G.J.

Abstract (from CDS):

The photon-dominated region (PDR) associated with the NGC 1977 molecular cloud has been observed at high resolution in the 13CO and C18O J=2-1 and the [CI] 3P1-3P0 lines. The N(13CO)/N(C18O) ratio has been plotted against visual extinction (Aν) and fits a power law relation. The highest values, as expected, occur for observed positions with the lowest derived extinction, with N(13CO)/N(C18O) exceeding the terrestrial value (5.5) for Aν≤60 magnitudes. In the outermost parts of the cloud (Aν≤20 magnitudes) the N(13CO)/N(C18O) ratio is largest, up to 20. Comparison with similar observations of the S140 and Orion Bright Bar regions implies that higher incident UV field leads to increased fractionation effects. The N(CI)/N(CO) ratio has been plotted against visual extinction, as derived from N(C18O), for the range Aν=20-100 magnitudes and also fits a power law relation. N(CI)/N(CO) increases with decreasing extinction from ∼0.03-0.04 for Aν∼100 mags. to ≥0.1 for Aν∼20 mags., corresponding to positions near the edge of the HII region/molecular cloud interface. Comparison with identical observations of the S140 and Orion Bright Bar regions implies that, unlike N(13CO)/N(C18O), the behaviour of N(CI)/N(CO) is insensitive to incident UV field over this range of extinction.

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Journal keyword(s): stars early-type - interstellar medium: HII regions - jets and outflows

Simbad objects: 6

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Number of rows : 6
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 1977 OpC 05 35 12.7 -04 48 21           ~ 256 0
2 [RLK73] IRc 2 IR 05 35 14.51548 -05 22 30.5943           ~ 673 1
3 NAME Orion Bright Bar reg 05 35 22.30 -05 24 33.0           ~ 1004 0
4 * c Ori Y*O 05 35 23.1646530684 -04 50 18.059784995 3.46 4.40 4.59 4.67 4.85 B1V+? 232 0
5 SH 2-140 OpC 22 19 07.8 +63 17 07           ~ 668 2
6 IRAS 22176+6303 Y*O 22 19 18.23 +63 18 47.5           ~ 600 0

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