J/A+A/570/A65   ATLASGAL massive clumps CO depletion         (Giannetti+, 2014)

ATLASGAL-selected massive clumps in the inner Galaxy. I. CO depletion and isotopic ratios. Giannetti A., Wyrowski F., Brand J., Csengeri T., Fontani F., Walmsley C.M., Nguyen Luong Q., Beuther H., Schuller F., Guesten R., Menten K.M. <Astron. Astrophys., 570, A65-65 (2014)> =2014A&A...570A..65G 2014A&A...570A..65G
ADC_Keywords: Molecular clouds ; Interstellar medium Keywords: ISM: abundances - ISM: clouds - ISM: molecules Abstract: In the low-mass regime, molecular cores have spatially resolved temperature and density profiles allowing a detailed study of their chemical properties. It is found that the gas-phase abundances of C-bearing molecules in cold starless cores rapidly decrease with increasing density. Here the molecules tend to stick to the grains, forming ice mantles. We study CO depletion in a large sample of massive clumps, and investigate its correlation with evolutionary stage and with the physical parameters of the sources. Moreover, we study the gradients in [12C]/[13C] and [18O]/[17O] isotopic ratios across the inner Galaxy, and the virial stability of the clumps. From the ATLASGAL 870µm survey we selected 102 clumps, which have masses in the range ∼102-3x104M, sampling different evolutionary stages. We use low-J emission lines of CO isotopologues and the dust continuum emission to infer the depletion factor fD. RATRAN one-dimensional models were also used to determine fD and to investigate the presence of depletion above a density threshold. The isotopic ratios and optical depth were derived with a Bayesian approach. We find a significant number of clumps with a high degree of CO depletion, up to ∼20. Larger values are found for colder clumps, thus for earlier evolutionary phases. For massive clumps in the earliest stages of evolution we estimate the radius of the region where CO depletion is important to be a few tenths of a pc. The value of the [12C]/[13C] ratio is found to increase with distance from the Galactic centre, with a value of ∼66±12 for the solar neighbourhood. The [18O]/[17O] ratio is approximately constant (∼4) across the inner Galaxy between 2kpc and 8kpc, albeit with a large range (∼2-6). Clumps are found with total masses derived from dust continuum emission up to ∼20 times higher than Mvir, especially among the less evolved sources. These large values may in part be explained by the presence of depletion: if the CO emission comes mainly from the low-density outer layers, the molecules may be subthermally excited, leading to an overestimate of the dust masses. CO depletion in high-mass clumps seems to behave as in the low-mass regime, with less evolved clumps showing larger values for the depletion than their more evolved counterparts, and increasing for denser sources. The ratios [12C]/[13C] and [18O]/[17O] are consistent with previous determinations, and show a large intrinsic scatter. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 100 35 Distances and classification for the sources in subsample S1, derived from C17O(3-2) tablea2.dat 100 44 Distances and classification for the sources in subsample S2, derived from C17O(3-2) tablea3.dat 100 23 Distances and classification for the sources in subsample S3, derived from C17O(3-2) tablea4.dat 91 43 Line parameters of of C17O(1-0) and C17O(3-2) for subsample S1 tablea5.dat 58 43 Line parameters of C18O(1-0) for subsample S1 tablea6.dat 58 43 Line parameters of 13CO(1-0) for subsample S1 tablea7.dat 58 43 Line parameters of 13C18O(1-0) for subsample S1 tablea8.dat 118 51 Line parameters of C18O(2-1) and C17O(3-2) for subsample S2 tablea9.dat 118 23 Line parameters of C17O(3-2) for subsample S3 tablea10.dat 41 43 Excitation temperature for subsample S1 tablea11.dat 41 51 Excitation temperature for subsample S2 tablea12.dat 97 43 Optical depths and isotopic ratios for subsample S1 tablea13.dat 103 43 Molecular column densities for subsample S1 (12C18O, 12C17O,1-0, 12C17O,3-2, 13C18O, N2) tablea14.dat 68 51 Molecular column densities for subsample S2 (12C18O, 12C17O, H2) tablea15.dat 51 23 Molecular column densities for subsample S3 (12C17O, H2) tablea16.dat 60 35 Masses from 870um dust emission and virial masses for subsample S1 tablea17.dat 60 44 Masses from 870um dust emission and virial masses for subsample S2 tablea18.dat 60 23 Masses from 870um dust emission and virial masses for subsample S3 -------------------------------------------------------------------------------- See also: J/MNRAS/443/1555 : ATLASGAL massive star forming clumps sample (Urquhart+ 2014) Byte-by-byte Description of file: tablea1.dat tablea2.dat tablea3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 20- 21 I2 h RAh Right ascension (J2000) 23- 24 I2 min RAm Right ascension (J2000) 26- 30 F5.2 s RAs Right ascension (J2000) 32 A1 --- DE- Declination sign (J2000) 33- 34 I2 deg DEd Declination (J2000) 36- 37 I2 arcmin DEm Declination (J2000) 39- 43 F5.2 arcsec DEs Declination (J2000) 44- 50 F7.2 km/s VLSR LSR velocity 52- 55 F4.1 kpc Dnear Near distance 57- 62 F6.1 pc znear Height above the Galactic plane for the near distance 64- 67 F4.1 kpc Dfar ?=- Far distance 69- 74 F6.1 pc zfar ?=- Height above the Galactic plane for the far distance 76 A1 --- HI [TNF-] Distance ambiguity resolution from Wienen et al., in prep: T=tangent, N=near, F=far 78- 81 F4.1 kpc Dlit ?=- Literature values for the distance 83- 84 I2 --- r_Dlit ? Reference for Dlit (2) 86- 87 A2 --- Met Method Method with which the distance Dlit was determined (3) 89- 92 F4.1 kpc Dist Adopted distance 94- 96 F3.1 kpc DGC Resulting Galactocentric distance 98-100 A3 --- Group Source classification (G1) -------------------------------------------------------------------------------- Note (2): References as follows: 1 = Caswell et al., (1975A&A....45..239C 1975A&A....45..239C) 2 = Green & McClure-Griffith (2011MNRAS.417.2500G 2011MNRAS.417.2500G) 3 = Moises et al. (2011MNRAS.411..705M 2011MNRAS.411..705M, Cat. J/MNRAS/411/705) 4 = Bik et al. (2005A&A...440..121B 2005A&A...440..121B, Cat. J/A+A/440/121) 5 = Sato et al. (2010PASJ...62..287S 2010PASJ...62..287S) 6 = Gwinn et al. (1992ApJ...393..149G 1992ApJ...393..149G, Cat. J/ApJ/393/149) 7 = Immer et al. (2012A&A...548A.120I 2012A&A...548A.120I) 8 = Xu et al. (2011ApJ...733...25X 2011ApJ...733...25X) 9 = Kurayama et al. (2011PASJ...63..513K 2011PASJ...63..513K) 10 = Pandian et al. (2008A&A...489.1175P 2008A&A...489.1175P) 11 = Sewilo et al. (2004ApJS..154..553S 2004ApJS..154..553S, Cat. J/ApJS/154/553) 12 = Bica et al. (2004MNRAS.352..226B 2004MNRAS.352..226B) 13 = Busfield et al. (2006MNRAS.366.1096B 2006MNRAS.366.1096B, Cat. J/MNRAS/366/1096) 14 = Urquhart et al. (2011MNRAS.410.1237U 2011MNRAS.410.1237U, Cat. J/MNRAS/410/1237) 15 = Figueredo et al. (2005AJ....129.1523F 2005AJ....129.1523F) 16 = Zhang et al. (2009ApJ...693..419Z 2009ApJ...693..419Z) 17 = Xu et al. (2009A&A...507.1117X 2009A&A...507.1117X) Note (3): Methods as follows: PA = Direct parallax measurement SP = Spectrophotometric measurement Hi = Hi self-absorption FR = Formaldehyde self-absorption -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea4.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/3]? Multiplicity index on Source 22- 26 F5.2 K.km/s T.dV1 C17O(1-0) integrated flux 28- 31 F4.2 K Tmb1 C17O(1-0) main beam temperature 33- 36 F4.2 K e_Tmb1 C17O(1-0) rms noise 38- 43 F6.2 km/s VLSR1 C17O(1-0) LSR velocity 45- 48 F4.2 km/s e_VLSR1 rms uncertainty on VLSR1 50- 52 F3.1 km/s DV1 C17O(1-0) δV 54- 56 F3.1 km/s e_DV1 rms uncertainty on DV1 58- 61 F4.1 K.km/s T.dV2 ?=- C17O(3-2) integrated flux 63- 66 F4.1 K Tmb2 ?=- C17O(3-2) main beam temperature 68- 71 F4.2 K e_Tmb2 C17O(3-2) rms noise 73- 78 F6.2 km/s VLSR2 ?=- C17O(3-2) LSR velocity 80- 83 F4.2 km/s e_VLSR2 ?=- rms uncertainty on VLSR2 85- 87 F3.1 km/s DV2 ?=- C17O(3-2) δV 89- 91 F3.1 km/s e_DV2 ?=- rms uncertainty on DV2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea5.dat tablea6.dat tablea7.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/3]? Multiplicity index on Source 22- 27 F6.2 K.km/s T.dV ?=- CO(1-0) isotope integrated flux 29- 33 F5.2 K Tmb ?=- CO(1-0) isotope main beam temperature 35- 38 F4.2 K e_Tmb CO(1-0) isotope rms noise 40- 45 F6.2 km/s VLSR ?=- CO(1-0) isotope LSR velocity 47- 50 F4.2 km/s e_VLSR ?=- rms uncertainty on VLSR 52- 54 F3.1 km/s DV ?=- CO(1-0) isotope δV 56- 58 F3.1 km/s e_DV ?=- rms uncertainty on DV -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea8.dat tablea9.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/4]? Multiplicity index on Source 22- 27 F6.2 K.km/s T.dV1 ? C18O(2-1) integrated flux 29- 33 F5.2 K Tmb1 ? C18O(2-1) main beam temperature 35- 38 F4.2 K rms1 ? C18O(2-1) rms noise 40- 46 F7.2 km/s VLSR1 ? C18O(2-1) LSR velocity 48- 51 F4.2 km/s e_VLSR1 ? rms uncertainty on VLSR1 53- 56 F4.1 km/s DV1 ? C18O(2-1) δV 58- 60 F3.1 km/s e_DV1 ? rms uncertainty on DV1 62- 64 F3.1 --- tau1 ? C18O(2-1) optical depth 66- 68 F3.1 --- b_tau2 ? Lower value of 68% confidence level of C18O(2-1) optical depth 69 A1 --- --- [-] 70- 72 F3.1 --- B_tau2 ? Upper value of 68% confidence level of C18O(2-1) optical depth 74- 78 F5.2 K.km/s T.dV2 ?=- C17O(3-2) integrated flux 80- 84 F5.2 K Tmb2 ?=- C17O(3-2) main beam temperature 86- 89 F4.2 K e_Tmb2 C17O(3-2) rms noise 91- 97 F7.2 km/s VLSR2 ?=- C17O(3-2) LSR velocity 99-102 F4.2 km/s e_VLSR2 ?=- rms uncertainty on VLSR2 104-106 F3.1 km/s DV2 ?=- C17O(3-2) δV 108-110 F3.1 km/s e_DV2 ?=- rms uncertainty on DV2 112-114 F3.1 --- tau2 ?=- C17O(3-2) Optical depth 116-118 F3.1 --- e_tau2 ?=- rms uncertainty on tau2 -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea10.dat tablea11.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/4]? Multiplicity index on Source 23- 26 F4.1 K Tex Excitation temperature 28- 31 F4.1 K b_Tex Lower value of 68% confidence level of Tex 32 A1 --- --- [-] 33- 36 F4.1 K B_Tex Upper value of 68% confidence level of Tex 37 A1 --- n_Tex [*] Note on Tex (1) 38- 40 A3 --- Group Group (G1) 41 A1 --- n_Group [)] ')' indicates classification of the main component -------------------------------------------------------------------------------- Note (1): For source AGAL015.029-00.669-2, the published value was a typo and the corrected value is tabulated, from the author. -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea12.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/3]? Multiplicity index on Source 23 A1 --- l_tau1 Limit flag on tau1 24- 27 F4.2 --- tau1 C18O(1-0) optical depth 29- 32 F4.2 --- b_tau1 ? Lower value of 68% confidence level of tau1 33 A1 --- --- [-] 34- 37 F4.2 --- B_tau1 ? Upper value of 68% confidence level of tau1 39 A1 --- l_tau2 Limit flag on tau2 40- 43 F4.2 --- tau2 C17O(1-0) optical depth 45- 48 F4.2 --- b_tau2 ? Lower value of 68% confidence level of tau2 49 A1 --- --- [-] 50- 53 F4.2 --- B_tau2 ? Upper value of 68% confidence level of tau2 55- 57 F3.1 --- 18/17O Isotopic ratio [18O]/[17O] 59- 61 F3.1 --- b_18/17O Lower value of 68% confidence level of isotopic ratio [18O]/[17O] 62 A1 --- --- [-] 63- 65 F3.1 --- B_18/17O Upper value of 68% confidence level of isotopic ratio [18O]/[17O] 67- 71 F5.1 --- 12/13C Isotopic ratio [12C]/[13C] 73- 76 F4.1 --- b_12/13C Lower value of 68% confidence level of isotopic ratio [12C]/[13C] 77 A1 --- --- [-] 78- 82 F5.1 --- B_12/13C Upper value of 68% confidence level of isotopic ratio [12C]/[13C] 84- 87 F4.1 --- 1217/1318 Isotopic ratio [12C17O]/[13C18O] 89- 92 F4.1 --- b_1217/1318 Lower value of 68% confidence level of isotopic ratio [12C17O]/[13C18O] 93 A1 --- --- [-] 94- 97 F4.1 --- B_1217/1318 Upper value of 68% confidence level of isotopic ratio [12C17O]/[13C18O] -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea13.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/3]? Multiplicity index on Source 22- 25 F4.1 10+16cm-2 N(CO) 12C18O molecular column density 27- 30 F4.1 10+16cm-2 b_N(CO) Lower value of 68% confidence level of N(12C18O) 31 A1 --- --- [-] 32- 35 F4.1 10+16cm-2 B_N(CO) Upper value of 68% confidence level of N(12C18O) 37- 40 F4.1 10+15cm-2 N(1-0) 12C17O molecular column density 42- 45 F4.1 10+15cm-2 b_N(1-0) Lower value of 68% confidence level of N(12C17O,1-0) 46 A1 --- --- [-] 47- 50 F4.1 10+15cm-2 B_N(1-0) Upper value of 68% confidence level of N(12C17O,1-0) 52 A1 --- l_N(3-2) Limit flag on N(12C17O3-2) 53- 56 F4.1 10+15cm-2 N(3-2) 12C17O molecular column density 58- 61 F4.1 10+15cm-2 b_N(3-2) ? Lower value of 68% confidence level of N(12C17O,3-2) 62 A1 --- --- [-] 63- 66 F4.1 10+15cm-2 B_N(3-2) ? Upper value of 68% confidence level of N(12C17O,3-2) 68 A1 --- l_N(1318) Limit flag on N(13C18O) 69- 73 F5.1 10+13cm-2 N(1318) 13C18O molecular column density 75- 79 F5.1 10+13cm-2 b_N(1318) ? Lower value of 68% confidence level of N(13C18O) 80 A1 --- --- [-] 81- 85 F5.1 10+13cm-2 B_N(1318) ? Upper value of 68% confidence level of N(13C18O) 87- 89 F3.1 10+23cm-2 N(H2) ? H2 molecular column density 91- 93 F3.1 10+23cm-2 b_N(H2) ? Lower value of 68% confidence level of N(H2) 94 A1 --- --- [-] 95- 98 F4.1 10+23cm-2 B_N(H2) ? Upper value of 68% confidence level of N(H2) 100-102 A3 --- Group Group (G1) 103 A1 --- n_Group [)] ')' indicates classification of the main component -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea14.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/4]? Multiplicity index on Source 22- 25 F4.1 10+16cm-2 N(CO) 12C18O molecular column density 27- 30 F4.1 10+16cm-2 b_N(CO) Lower value of 68% confidence level of N(12C18O) 31 A1 --- --- [-] 32- 35 F4.1 10+16cm-2 B_N(CO) Upper value of 68% confidence level of N(12C18O) 37 A1 --- l_N(1217) Limit flag on N(12C17O) 38- 41 F4.1 10+15cm-2 N(1217) 12C18O molecular column density 43- 46 F4.1 10+15cm-2 b_N(1217) ? Lower value of 68% confidence level of N(12C17O) 47 A1 --- --- [-] 48- 51 F4.1 10+15cm-2 B_N(1217) ? Upper value of 68% confidence level of N(12C17O) 53- 55 F3.1 10+23cm-2 N(H2) ? H2 molecular column density 57- 59 F3.1 10+23cm-2 b_N(H2) ? Lower value of 68% confidence level of N(H2) 60 A1 --- --- [-] 61- 63 F3.1 10+23cm-2 B_N(H2) ? Upper value of 68% confidence level of N(H2) 65- 67 A3 --- Group Group (G1) 68 A1 --- n_Group [)] ')' indicates classification of the main component -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea15.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 20- 23 F4.1 10+15cm-2 N(1217) 12C17O molecular column density 25- 28 F4.1 10+15cm-2 b_N(1217) Lower value of 68% confidence level of N(12C17O) 29 A1 --- --- [-] 30- 33 F4.1 10+15cm-2 B_N(1217) Upper value of 68% confidence level of N(12C17O) 35- 38 F4.1 10+23cm-2 N(H2) H2 molecular column density 40- 42 F3.1 10+23cm-2 b_N(H2) Lower value of 68% confidence level of N(H2) 43 A1 --- --- [-] 44- 47 F4.1 10+23cm-2 B_N(H2) Upper value of 68% confidence level of N(H2) 49- 51 A3 --- Group Group (G1) -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea16.dat tablea17.dat tablea18.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- --- [AGAL] 5- 18 A14 --- AGAL AGAL source name (LLLL.lll+BB.bbb) 19 A1 --- --- [-] 20 I1 --- m_AGAL [1/3]? Multiplicity index on Source 22- 26 F5.2 10+3Msun Mass Mass 28- 32 F5.2 10+3Msun b_Mass Lower value of 68% confidence level of Mass 33 A1 --- --- [-] 34- 38 F5.2 10+3Msun B_Mass Upper value of 68% confidence level of Mass 40- 44 F5.2 10+3Msun Mvir Viral mass 46- 50 F5.2 10+3Msun b_Mvir Lower value of 68% confidence level of Mvir 51 A1 --- --- [-] 52- 56 F5.2 10+3Msun B_Mvir Upper value of 68% confidence level of Mvir 58- 60 A3 --- Group Group (G1) -------------------------------------------------------------------------------- Global notes: Note (G1): Groups as follows: D24 = 22 brightest sources that are dark at 24um D8 = 23 brightest objects dark at 8um IRB = 32 brightest sources of the whole survey, ex-cluding the Central Molecular Zone (i.e. the central few x102pc) RMS = 25 brightest sources, that are classified as a Massive Young Stellar Object (MYSO) in the Red MSX Sources survey (Urquhart et al., 2008A&A...487..253U 2008A&A...487..253U. J/A+A/487/253) -------------------------------------------------------------------------------- History: From electronic version of the journal Acknowledgements: Andrea Giannetti, agianne(at)ira.inaf.it
(End) Patricia Vannier [CDS] 02-Dec-2014
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