J/A+A/640/A74         SOLIS. VIII. L1157-B1 spectra            (Spezzano+, 2020)

Seeds of Life in Space (SOLIS). VIII. SiO isotopic fractionation and a new insight in the shocks of L1157-B1. Spezzano S., Codella C., Podio L., Ceccarelli C., Caselli P., Neri R., Lopez-Sepulcre A. <Astron. Astrophys. 640, A74 (2020)> =2020A&A...640A..74S 2020A&A...640A..74S (SIMBAD/NED BibCode)
ADC_Keywords: Radio lines ; Spectra, radio Keywords: ISM: clouds - ISM: molecules - ISM: jets and outflows Abstract: Contrary to what is expected from models of Galactic chemical evolution (GCE), the isotopic fractionation of silicon (Si) in the Galaxy has been recently found to be constant. This finding calls for new observations, also at cores scales, to re-evaluate the fractionation of Si. L1157-B1 is one of the outflow shocked regions along the blue-shifted outflow driven by the Class 0 protostar L1157-mm, and is an ideal laboratory to study the material ejected from the grains in very short timescales, i.e. its chemical composition is representative of the composition of the grains. We imaged 28SiO, 29SiO and 30SiO J = 2-1 emission towards L1157-B1 and B0 with the NOrthern Extended Millimeter Array (NOEMA) interferometer as part of the Seeds of Life in Space (SOLIS) large project. We present here a study of the isotopic fractionation of SiO towards L1157-B1. Furthermore, we use the high spectral resolution observations on the main isotopologue, 28SiO, to study the jet impact on the dense gas. We present here also single-dish observations obtained with the IRAM 30m telescope and Herschel-HIFI. We carried out a non-LTE analysis using a Large Velocity Gradient (LVG) code to model the single-dish observations. From our observations we can show that (i) the (2-1) transition of the main isotopologue is optically thick in L1157-B1 even at high velocities, and (ii) the [29SiO/30SiO] ratio is constant across the source, and consistent with the solar value of 1.5. We report the first isotopic fractionation maps of SiO in a shocked region and show the absence of a mass dependent fractionation in 29Si and 30Si across L1157-B1. A high-velocity bullet in 28SiO has been identified, showing the signature of a jet impacting on the dense gas. With the dataset presented in this paper, both interferometric and single-dish, we were able to study in great detail the gas shocked at the B1a position and its surrounding gas. Description: The single-dish observations of the 28SiO, 29SiO, and 30SiO lines from J=2-1 to J=8-7 (see Table 1 for the frequencies) have been obtained using the IRAM 30-m antenna in the context of the ASAI Large Program. Observations have been done in Wobbler Mode at the position of the B1 shock, namely at RA(2000)=20:39:10.02, DE(2000)=+68:01:10.5. The SiO, 29SiO, and 30SiO J=12-11 transitions were observed with Herschel-HIFI on 2010 October 27 and 2009 August 1, during the unbiased spectral survey CHESS (e.g. Ceccarelli et al. 2010) with the HIFI bands 1a, at the same position used for the IRAM 30-m observations. The 28SiO, 29SiO and 30SiO J=2-1 lines were observed with NOEMA using the Polyfix correlator, with a total spectral band of 8GHz, and a spectral resolution of 2.0MHz (7.3km/s). The main isotopologue has been observed also at high spectral resolution (62.5kHz, 0.22km/s), here smoothed to 0.5km/s (28SiO_HR.lmv-clean). Objects: ---------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------- 20 39 11 +68 01.3 L1157-B1 = [DE95] LDN 1157 B1 ---------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 110 4 List of fits datacubes listsp.dat 44 15 List of spectra fits/* . 4 Individual fits datacubes sp/* . 15 Individual spectra -------------------------------------------------------------------------------- See also: J/A+A/605/A57 : SOLIS. I. OMC2-FIR4 HC3N and HC5N images (Fontani+, 2017) J/A+A/605/L3 : SOLIS. II. L1157-B1 NH2CHO image (Codella+, 2017) J/A+A/640/A75 : SOLIS. X. NGC 1333 IRAS 4A images (De Simone+, 2020) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 9 F9.5 deg RAdeg Right Ascension of center (J2000) 10- 18 F9.5 deg DEdeg Declination of center (J2000) 20- 23 I4 --- Nx Number of pixels along X-axis 25- 28 I4 --- Ny Number of pixels along Y-axis 30- 32 I3 --- Nz Number of pixels along Z-axis 34- 42 F9.1 m/s bVRAD Lower value of VRAD interval 44- 49 I6 m/s BVRAD Upper value of VRAD interval 51- 58 F8.3 m/s dVRAD VRAD resolution 60- 65 I6 Kibyte size Size of FITS file 67- 84 A18 --- FileName Name of FITS file, in subdirectory fits 86-110 A25 --- Title Title of the FITS file -------------------------------------------------------------------------------- Byte-by-byte Description of file: listsp.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- FileName Name of the spectrum file in subdirectoy sp 18- 44 A27 --- Title Title of the file -------------------------------------------------------------------------------- Byte-by-byte Description of file: sp/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 15 F13.9 km/s Vlsr LSR velocity 19- 29 E11.5 K Tmb Mean brightness temperature -------------------------------------------------------------------------------- Acknowledgements: Silvia Spezzano, spezzano(at)mpe.mpg.de References: Fontani et al., Paper I 2017A&A...605A..57F 2017A&A...605A..57F, Cat. J/A+A/605/A57 Codella et al., Paper II 2017A&A...605L...3C 2017A&A...605L...3C, Cat. J/A+A/605/L3 Ceccarelli et al., 2017ApJ...850..176C 2017ApJ...850..176C Punanova et al., Paper III 2018ApJ...855..112P 2018ApJ...855..112P Favre et al., Paper IV 2018ApJ...859..136F 2018ApJ...859..136F Codella et al., Paper V 2020A&A...635A..17C 2020A&A...635A..17C Favre et al., Paper VII 2020A&A...635A.189F 2020A&A...635A.189F Feng et al., Paper IX 2020ApJ...896...37F 2020ApJ...896...37F De Simone et al., Paper X 2020A&A...640A..74D 2020A&A...640A..74D, Cat. J/A+A/640/A74
(End) Patricia Vannier [CDS] 10-Jun-2020
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