J/AJ/162/235  HST/STIS near-UV spectrum of η Telescopii  (Youngblood+, 2021)

A Radiatively Driven Wind from the ηTel Debris Disk Youngblood A., Roberge A., MacGregor M.A., Brandeker A., Weinberger A.J., Perez S., Grady C., Welsh B. <Astron. J., 162, 235 (2021)> =2021AJ....162..235Y 2021AJ....162..235Y
ADC_Keywords: Stars, A-type; Spectra, ultraviolet; Abundances Keywords: A stars ; Circumstellar matter ; Ultraviolet astronomy ; Protoplanetary disks Abstract: We present far- and near-ultraviolet absorption spectroscopy of the ∼23Myr edge-on debris disk surrounding the A0V star ηTelescopii, obtained with the Hubble Space Telescope Space Telescope Imaging Spectrograph. We detect absorption lines from CI, CII, OI, MgII, AlII, SiII, SII, MnII, FeII, and marginally NI. The lines show two clear absorption components at -22.7±0.5km/s and -17.8±0.7km/s, which we attribute to circumstellar (CS) and interstellar gas, respectively. CO absorption is not detected, and we find no evidence for star-grazing exocomets. The CS absorption components are blueshifted by -16.9±2.6km/s in the star's reference frame, indicating that they are outflowing in a radiatively driven disk wind. We find that the C/Fe ratio in the ηTel CS gas is significantly higher than the solar ratio, as is the case in the βPic and 49Cet debris disks. Unlike those disks, however, the measured C/O ratio in the ηTel CS gas is consistent with the solar value. Our analysis shows that because ηTel is an earlier type star than βPic and 49Cet, with more substantial radiation pressure at the dominant CII transitions, this species cannot bind the CS gas disk to the star as it does for βPic and 49Cet, resulting in the disk wind. Description: We observed the ηTel debris disk with Hubble Space Telecscope Space Telescope Imaging Spectrograph (HST/STIS) on 2016 October 3 and 2016 October 6. The wavelength coverage of the STIS spectra is 1164-1951Å and 2587-2851Å. The spectra were obtained with the E140H and E230H echelle gratings (grating settings i1271, c1416, c1598, i1813, and i2713), providing an average dispersion of λ/228000Å/pixel. Objects: ------------------------------------------------- RA (2000) DE Designation(s) ------------------------------------------------- 19 22 51.21 -54 25 26.1 * eta Tel = * eta Tel ------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fig1.dat 75 142094 Co-added spectrum of ηTelescopii from HST STIS E140H and E230H observations -------------------------------------------------------------------------------- See also: III/254 : 2nd Cat. Radial Velocities with Astrometric Data (Kharchenko+, 2007) I/345 : Gaia DR2 (Gaia Collaboration, 2018) I/345 : Gaia DR2 (Gaia Collaboration, 2018) J/ApJ/497/330 : Candidate main-sequence stars (Mannings+, 1998) J/AN/328/889 : Mean Radial Velocities of open clusters (Kharchenko+, 2007) J/ApJ/660/1556 : Characterization of dusty debris disks (Rhee+, 2007) J/AJ/143/134 : Candidate members of βPic/ABDor groups (McCarthy+, 2012) J/PASP/125/477 : Gas Survey of Protoplanetary Systems. I. (Dent+, 2013) J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013) J/ApJS/211/25 : Spitzer/IRS debris disk catalog. I. (Chen+, 2014) J/MNRAS/469/521 : CO, C & O gas content debris discs predictions (Kral+, 2017) J/A+A/614/A3 : 6 cold-gas-bearing debris-disc stars spectra (Rebollido+, 2018) J/ApJ/896/24 : Properties of atomic lines 51 Oph UV spectra (Jenkins+, 2020) J/A+A/639/A11 : Exocomets. A Spectroscopic Survey (Rebollido+, 2020) Byte-by-byte Description of file: fig1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 24 E24.18 0.1nm lambda [1163/2835] Wavelength, Angstroms 26- 50 E25.18 10mW/m2/nm Flux Flux Density, erg/cm2/s/Ang 52- 75 E24.18 10mW/m2/nm e_Flux Flux Density Error, erg/cm2/s/Ang -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 18-Feb-2022
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