J/other/Univ/10.465       FITS images of SAO 206462                 (Xie+, 2024)

Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): Dynamical evidence of a spiral-arm-driving and gap-opening protoplanet from SAO 206462 spiral motion. Xie C., Xie C., Ren B.B., Benisty M., Ginski C., Fang T., Casassus S., Bae J., Facchini S., Menard F., van Holstein R.G. <Universe, 10, 465 (2024)> =2024Univ....10.465X 2024Univ....10.465X (SIMBAD/NED BibCode)
ADC_Keywords: Stars, normal ; Interstellar medium ; Optical ; Infrared Keywords: protoplanetary disks - coronagraphic imaging - orbital motion - planetary system formation Abstract: In the early stages of planetary system formation, young exoplanets gravitationally interact with their surrounding environments and leave observable signature on protoplanetary disks. Among these structures, a pair of nearly symmetric spiral arms can be driven by a giant protoplanet. For the double-spiraled SAO 206462 protoplanetary disk, we obtained three epochs of observations spanning 7yr using the Very Large Telescope's SPHERE instrument in near-infrared J-band polarized light. By jointly measuring the motion of the two spirals at three epochs, we obtained a rotation rate of -0.85±0.05 deg per year. This rate corresponds to a protoplanet at 66±3au on a circular orbit dynamically driving both spirals. The derived location agrees with the gap in ALMA dust-continuum observations, indicating that the spiral driver may also carve the observed gap. What is more, a dust filament at ∼63 au observed by ALMA coincides with the predicted orbit of the spiral-arm-driving protoplanet. This double-spiraled system is an ideal target for protoplanet imaging. Description: FITS files of disk images in SPHERE/IRDIS (J-band) from the Very Large Telescope. The stars are located at the mathematical centers of the arrays. The units are in counts per pixel for Qphi data. Objects: ----------------------------------------------------- RA (2000) DE Designation(s) ----------------------------------------------------- 15 15 48.45 -37 09 16.02 SAO 206462 = HD 135344B ----------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 121 3 List of fits images fits/* . 3 Individual fits images -------------------------------------------------------------------------------- See also: J/A+A/560/A105 : SAO 206462 polarised Ks image (Garufi+, 2013) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Star name 12- 13 I2 h RAh Right Ascension of center (J2000) 15- 16 I2 min RAm Right Ascension of center (J2000) 18- 22 F5.2 s RAs Right Ascension of center (J2000) 24 A1 --- DE- Declination sign of center (J2000) 25- 26 I2 deg DEd Declination of center (J2000) 28- 29 I2 arcmin DEm Declination of center (J2000) 31- 35 F5.2 arcsec DEs Declination of center (J2000) 37- 39 I3 --- Nx Number of pixels along X-axis 41- 43 I3 --- Ny Number of pixels along Y-axis 45- 47 I3 Kibyte size Size of FITS file 49- 72 A24 --- FileName Name of FITS file, in subdirectory fits 74-121 A48 --- Title Title of the FITS file -------------------------------------------------------------------------------- Acknowledgements: Bin Ren, bin.ren(at)oca.eu
(End) Patricia Vannier [CDS] 18-Dec-2024
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line