Chemistry in disks I - Deep search for NH in the protoplanetary disks around LkCa 15, MWC 480, and DM Tau
arXiv:astro-ph/0612534 · doi:10.1051/0004-6361:20065385
Abstract
Aims: To constrain the ionization fraction in protoplanetary disks, we present new high-sensitivity interferometric observations of NH in three disks surrounding DM Tau, LkCa 15, and MWC 480. Methods: We used the IRAM PdBI array to observe the NH J=1-0 line and applied a -minimization technique to estimate corresponding column densities. These values are compared, together with HCO column densities, to results of a steady-state disk model with a vertical temperature gradient coupled to gas-grain chemistry. Results: We report two \ndhp detections for LkCa 15 and DM Tau at the level and an upper limit for MWC 480. The column density derived from the data for LkCa 15 is much lower than previously reported. The [NH/HCO] ratio is on the order of 0.02--0.03. So far, HCO remains the most abundant observed molecular ion in disks. Conclusions: All the observed values generally agree with the modelled column densities of disks at an evolutionary stage of a few million years (within the uncertainty limits), but the radial distribution of the molecules is not reproduced well. The low inferred concentration of NH in three disks around low-mass and intermediate-mass young stars implies that this ion is not a sensitive tracer of the overall disk ionization fraction.
arXiv comment10 pages, 6 figures
References in corpus (25)
- Accretion Disks Around Young Objects. II. Tests of Well-Mixed Models with Ism Dust
- Dynamical Masses of T Tauri Stars and Calibration of PMS Evolution
- Molecular ions in L1544. II. The ionization degree
- Organic molecules in protoplanetary disks around TTauri and HerbigAe stars
- Molecular Evolution in Collapsing Prestellar Cores III: Contraction of A Bonnor-Ebert Sphere
- Desorption rates and sticking coefficients for CO and N2 interstellar ices
- Imaging the Disk around TW Hya with the Submillimeter Array
- Molecular ions in L1544. I. Kinematics
- Submillimeter lines from circumstellar disks around pre-main sequence stars
- Resolving the inner dust disks surrounding LkCa 15 and MWC 480 at mm wavelengths
- Axi-symmetric models of ultraviolet radiative transfer with applications to circumstellar disk chemistry
- Comparative Chemistry of Diffuse Clouds II: CN, HCN, HNC, CH3CN & N2H+
- Reduction of chemical networks. II. Analysis of the fractional ionisation in protoplanetary discs
- A New Probe of the Planet-Forming Region in T Tauri Disks
- Continuum and CO/HCO+ Emission from the Disk Around the T Tauri Star LkCa 15
- Imaging chemical differentiation around the low-mass protostar L483-mm
- Gas-phase CO in protoplanetary disks: a challenge for turbulent mixing
- Estimation and reduction of the uncertainties in chemical models: Application to hot core chemistry
- Millimeter observations and modeling of the AB Aurigae system
- Interferometric Observations of Formaldehyde in the Protoplanetary Disk around LkCa15
- Deuterated H in proto-planetary disks
- Deuterated molecules in DM Tau: DCO+, but no HDO
- On the Influence of Uncertainties in Chemical Reaction Rates on Results of the Astrochemical Modelling
- Dynamical and chemical properties of the "starless" core L1014
- Line emission from circumstellar disks around A stars
Cited by in corpus (57)
- Protoplanetary Disks and Their Evolution
- A simple model for the evolution of the dust population in protoplanetary disks
- Our astrochemical heritage
- 2021 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules
- 2018 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules
- A dual-frequency sub-arcsecond study of proto-planetary disks at mm wavelengths: First evidence for radial variations of the dust properties
- Molecules with ALMA at Planet-forming Scales (MAPS) I: Program Overview and Highlights
- The cometary composition of a protoplanetary disk as revealed by complex cyanides
- Chemistry in Disks. IV. Benchmarking gas-grain chemical models with surface reactions
- Constraining the X-ray and Cosmic Ray Ionization Chemistry of the TW Hya Protoplanetary Disk: Evidence for a Sub-interstellar Cosmic Ray Rate
- Chemical Processes in Protoplanetary Disks
- Chemical evolution of turbulent protoplanetary disks and the Solar nebula
- Disk Imaging Survey of Chemistry with SMA: II. Southern Sky Protoplanetary Disk Data and Full Sample Statistics
- Disk Imaging Survey of Chemistry with SMA (DISCS): I. Taurus Protoplanetary Disk Data
- Detecting Weak Spectral Lines in Interferometric Data through Matched Filtering
- H2CO and N2H+ in Protoplanetary Disks: Evidence for a CO-ice Regulated Chemistry
- Photodissociation of interstellar N2
- Rotating molecular outflows: the young T Tauri star in CB26
- Consistent dust and gas models for protoplanetary disks III. Models for selected objects from the FP7 DIANA project
- Chemistry in Protoplanetary Disks: A Sensitivity Analysis
- Chemistry in Disks. III. -- Photochemistry and X-ray driven chemistry probed by the ethynyl radical (CCH) in DM Tau, LkCa 15, and MWC 480
- Protoplanetary Disk Structure With Grain Evolution: the ANDES Model
- Consistent dust and gas models for protoplanetary disks: II. Chemical networks and rates
- Chemistry in disks. XI. Sulfur-bearing species as tracers of protoplanetary disk physics and chemistry: the DM Tau case
- The masses of young stars: CN as a probe of dynamical masses
- First detection of c-C3H2 in a circumstellar disk
- Chemistry in Disks X: The Molecular Content of Proto-planetary Disks in Taurus
- CID: Chemistry in disks VI.sulfur-bearing molecules in the protoplanetary disks surrounding LkCa15, MWC480, DM Tau, and GO Tau
- Chemistry in Disks. IX. Observations and modeling of HCO+ and DCO+ in DM Tau
- First detection of gas-phase ammonia in a planet-forming disk
- Chemistry in Disks. V: CN and HCN in proto-planetary disks
- Impact of grain evolution on the chemical structure of protoplanetary disks
- The Distribution and Chemistry of HCO in the DM Tau Protoplanetary Disk
- Stellar energetic particle ionization in protoplanetary disks around T Tauri stars
- Stacking Spectra in Protoplanetary Disks: Detecting Intensity Profiles from Hidden Molecular Lines in HD 163296
- Molecular line radiative transfer in protoplanetary disks: Monte Carlo simulations versus approximate methods
- An unbiased ALMA spectral survey of the LkCa 15 and MWC 480 protoplanetary disks
- The chemistry of disks around T Tauri and Herbig Ae/Be stars
- Chemistry in a gravitationally unstable protoplanetary disc
- Millimeter Observations of the Transition Disk around HD135344B (SAO 206462)
- Molecular line emission from a protoplanetary disk irradiated externally by a nearby massive star
- The CN/C15 N isotopic ratio towards dark clouds
- H2CO distribution and formation in the TW Hya disk
- The Ionization Fraction in the DM Tau Protoplanetary Disk
- Chemical and thermal structure of protoplanetary disks as observed with ALMA
- The Effects of Initial Abundances on Nitrogen in Protoplanetary Disks
- X-ray radiative transfer in protoplanetary disks - The role of dust and X-ray background fields
- Molecular content of the circumstellar disk in AB Aur: First detection of SO in a circumstellar disk
- Chemical composition of the circumstellar disk around AB Aurigae
- Protoplanetary disks: Sensitivity of the chemical composition to various model parameters
- HS observations in young stellar disks in Taurus
- An Unbiased 1.3 mm Emission Line Survey of the Protoplanetary Disk Orbiting LkCa 15
- Modeling Time Dependent Water Chemistry Due to Powerful X-ray Flares from T-Tauri Stars
- PRODIGE -- Planet-forming disks in Taurus with NOEMA. I. Overview and first results for 12CO, 13CO, and C18O
- Chemical evolution of a protoplanetary disk
- Chemistry in protoplanetary disks (short review in Russian)
- Protoplanetary Disk Chemistry