Revisiting the Helium and Hydrogen Accretion Indicators at TWA 27B: Weak Mass Flow at Near-Freefall Velocity
arXiv:2401.04763 · doi:10.3847/1538-4357/ad1ee9
Abstract
TWA 27B (2M1207b) is the first directly-imaged planetary-mass (MP ~ 5 MJ) companion (Chauvin et al. 2004) and was observed at 0.9--5.3 micron with JWST/NIRSpec (Luhman et al. 2023). To understand the accretion properties of TWA 27B, we search for continuum-subtracted near-infrared helium and hydrogen emission lines and measure their widths and luminosities. We detect the He I triplet at 4.3 sigma and all Paschen-series lines covered by NIRSpec (Pa alpha, Pa beta, Pa gamma, Pa delta) at 4--5 sigma. The three brightest Brackett-series lines (Br alpha, Br beta, Br gamma) as well as Pf gamma and Pf delta are tentative detections at 2--3 sigma. We provide upper limits on the other hydrogen lines, including on H alpha through Hubble Space Telescope archival data. Three lines can be reliably deconvolved to reveal an intrinsic width Delta v = 67+-9 km/s, which is 60% of the surface freefall velocity. The line luminosities seem significantly too high to be due to chromospheric activity. Converting line luminosities to an accretion rate yields Mdot ~ 5e-9 MJ/yr when using scaling relationships for planetary masses, and Mdot ~ 0.1e-9 MJ/yr with extrapolated stellar scalings. Several of these lines represent first detections at an accretor of such low mass. The weak accretion rate implies that formation is likely over. This analysis shows that JWST can be used to measure low line-emitting mass accretion rates onto planetary-mass objects, motivates deeper searches for the mass reservoir feeding TWA 27B, and hints that other young directly-imaged objects might -- hitherto unbeknownst -- also be accreting.
arXiv commentIn press at ApJ. Main text: 10 pages, 5 figures, 1 table, 1 equation. Appendix: 12 figures (line profiles). Comments welcome. v2: added one reference. v3: added RV velocity (probable systemic velocity) of primary to Fig. 3b. v4: no change, only added DOI of open-access, published version (2024 March 18)
References in corpus (53)
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- Images of a fourth planet orbiting HR 8799
- A Giant Planet Candidate near a Young Brown Dwarf
- The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilities
- The James Webb Space Telescope Mission
- Two accreting protoplanets around the young star PDS 70
- X-Shooter spectroscopy of young stellar objects in Lupus: Accretion properties of class II and transitional objects
- Accretion in Brown Dwarfs: an Infrared View
- X-Shooter spectroscopy of young stellar objects: IV -- Accretion in low-mass stars and sub-stellar objects in Lupus
- The T Tauri Phase Down to Nearly Planetary Masses: Echelle Spectra of 82 Very Low Mass Stars and Brown Dwarfs
- Population Properties of Brown Dwarf Analogs to Exoplanets
- Predicting the Properties of Binary Stellar Systems: The Evolution of Accreting Protobinary Systems
- Distribution of Accreting Gas and Angular Momentum onto Circumplanetary Disks
- The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope III. Integral-field spectroscopy
- The Far-Ultraviolet Spectra of TW Hya. II. Models of H2 Fluorescence in a Disk
- Population-Level Eccentricity Distributions of Imaged Exoplanets and Brown Dwarf Companions: Dynamical Evidence for Distinct Formation Channels
- The Planetary Mass Companion 2MASS1207-3932 B: Temperature, Mass and Evidence for an Edge-On Disk
- Magellan Adaptive Optics Imaging of PDS 70: Measuring the Mass Accretion Rate of a Young Giant Planet within a Gapped Disk
- X-Shooter spectroscopy of young stellar objects: II. Impact of chromospheric emission on accretion rate estimates
- Circumbinary Accretion from Finite and Infinite Disks
- Protoplanetary Disk Masses from Stars to Brown Dwarfs
- Measuring Protoplanetary Disk Accretion with H I Pf-beta
- Modeling T Tauri Winds from He I 10830 Profiles
- Evidence Against an Edge-On Disk Around the Extrasolar Planet 2MASS 1207 b and a New Thick Cloud Explanation for its Under-Luminosity
- Measuring tiny mass accretion rates onto young brown dwarfs
- Theoretical Model of Hydrogen Line Emission from Accreting Gas Giants
- Redshifted Absorption at He I 10830 as a Probe of the Accretion Geometry of T Tauri Stars
- A Widely-Separated, Highly-Occluded Companion to the Nearby Low-Mass T Tauri Star TWA 30
- An extensive VLT/X-Shooter library of photospheric templates of pre-main sequence stars
- Hubble and Spitzer Observations of an Edge-on Circumstellar Disk around a Brown Dwarf
- Magnetospheric Accretion as a Source of H Emission from Proto-planets around PDS 70
- GIARPS High-resolution Observations of T Tauri stars (GHOsT). IV. Accretion properties of the Taurus-Auriga young association
- The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits. III. The frequency of brown dwarfs and giant planets as companions to solar-type stars
- Comparison of planetary Hα-emission models: A new correlation with accretion luminosity
- X-shooter spectroscopy of young stars with disks. The TW Hydrae association as a probe of the final stages of disk accretion
- Constraints on the formation mechanism of the planetary mass companion of 2MASS 1207334-393254
- Strong H emission and signs of accretion in a circumbinary planetary mass companion from MUSE
- Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H alpha
- JWST/NIRSpec Observations of the Planetary Mass Companion TWA 27B
- A Census of the TW Hya Association with Gaia
- Near-infrared Accretion Signatures from the Circumbinary Planetary Mass Companion Delorme 1 (AB)b
- Emission line variability of young 10-30 Mjup companions : I. The case of GQ Lup b and GSC 06214-00210 b
- The Planetary Luminosity Problem: "Missing Planets" and the Observational Consequences of Episodic Accretion
- ALMA Observations of the Young Substellar Binary System 2M1207
- A Census of the Low Accretors. I: The Catalog
- Resolved near-UV hydrogen emission lines at 40-Myr super-Jovian protoplanet Delorme 1 (AB)b: Indications of magnetospheric accretion
- The Planetary Accretion Shock. III. Smoothing-free 2.5D simulations and calculation of H alpha emission
- An ALMA Survey for Disks Orbiting Low-Mass Stars in the TW Hya Association
- The Late-Type Extension to MoVeRS (LaTE-MoVeRS): Proper motion verified low-mass stars and brown dwarfs from SDSS, 2MASS, and WISE
- Comparing Apples with Apples: Robust Detection Limits for Exoplanet High-Contrast Imaging in the Presence of non-Gaussian Noise
- The He I 10830 line as a probe of winds and accretion in young stars in Lupus and Upper Scorpius
- 2MASS J11151597+1937266: A Young, Dusty, Isolated, Planetary-Mass Object with a Potential Wide Stellar Companion
- Planetary line-to-accretion luminosity scaling relations: Extrapolating to higher-order hydrogen lines
Cited by in corpus (6)
- Analyzing JWST/NIRSpec Hydrogen Line Detections at TWA 27B: Constraining Accretion Properties and Geometry
- Multi-frequency observations of PDS 70c: Radio emission mechanisms in the circum-planetary environment
- JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD
- Occurrence rates of accreting companions from a new method for computing emission-line survey sensitivity: application to the H-alpha Giant Accreting Protoplanet Survey
- Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint
- Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets