J/A+A/621/A50           TX Psc ALMA CO(2-1) images              (Brunner+, 2019)

ALMA observations of the "fresh" carbon-rich AGB star TX Piscium. The discovery of an elliptical detached shell. Brunner M., Mecina M., Maercker M., Dorfi E.A., Kerschbaum F., Olofsson H., Rau G. <Astron. Astrophys. 621, A50 (2019)> =2019A&A...621A..50B 2019A&A...621A..50B (SIMBAD/NED BibCode)
ADC_Keywords: Stars, carbon ; Stars, late-type ; Carbon monoxide Keywords: stars: AGB and post-AGB - stars: carbon - stars: evolution - stars: mass-loss - stars: late-type Abstract: We observed the carbon-rich asymptotic giant branch (AGB) star TX Piscium (TX Psc) with ALMA in CO(2-1) emission to investigate the circumstellar envelope (CSE) and mass-loss history of this object. Previous observations with Herschel in the far infrared have shown a ring-like structure in dust emission (2011A&A...532A.135J 2011A&A...532A.135J). Our molecular gas observations of the CO(2-1) emission line cover this structure with significantly higher spatial resolution to investigate its origin. Description: The datacubes show the CO(2-1) gas distribution in the CSE of TX Psc as observed by ALMA with the main array (12 antennas) and the Atacama Compact Array (ACA, 7m antennas). The images have been created with CASA by face-to-face support of the Nordic ARC Node and give mosaics with a size of 45"x45" and a resolution of 1" for the main array and a beamsize of 7.6"x 4.44" for the ACA. The spectral resolution is 0.65km/s (499.84kHz) for he CO(2-1) line at a frequency of rest of 230.538GHz. The stellar velocity is roughly at 13km/s, marking the center velocity. In both datacubes two components are detected in the CSE: a strong and compact present-day wind close to the stellar position, and a larger shell structure with a maximum radius of roughly 17", which is of elliptical shape. Similar detached shell structures are usually detected only with spherical shapes, while the axis ratio of our elliptical shell is 1.3 and therefore shows a clear deviation from spherical symmetry. Objects: ------------------------------------------------ RA (2000) DE Designation(s) ------------------------------------------------ 23 46 23.51 +03 29 12.5 TX Psc = * 19 Psc ------------------------------------------------ File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 164 2 List of fits images fits/* . 2 Individual fits images -------------------------------------------------------------------------------- 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- 22 I3 --- Nx Number of pixels along X-axis 24- 26 I3 --- Ny Number of pixels along Y-axis 28- 53 A26 "datime" Obs.date Onservations date (YYYY-MM-DDTHH:MM:SS.ssssss) 55- 61 F7.3 GHz bFreq [230.516] Lower value of frequency interval 63- 69 F7.3 GHz BFreq [230.538] Upper value of frequency interval 71- 76 I6 Hz dFreq [499845] Frequency resolution 78- 82 I5 Kibyte size [47118] Size of FITS file 84-113 A30 --- FileName Name of FITS file, in subdirectory fits 115-164 A50 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Magdalena Brunner, magdalena.brunner(at)univie.ac.at
(End) Patricia Vannier [CDS] 12-Nov-2018
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