Kay Justtanont
Kays forskning fokuseras kring att studera rymddamm och gas runt sent utvecklade stjärnor, så kallade AGB-stjärnor. Mycket av Kays arbete involverar modellerande av markbaserade observationer samt data från olika astronomiska rymduppdrag. Kay är också intresserad av rymddamm i stjärnbildande regioner och utflöde från unga stellära objekt.
Kay arbetar för tillfället med det mid-infraröda instrumentet (MIRI) som svensk projekassistent. MIRI är ett av fyra instrument som ska flyga med James Webb Space Telescope (JWST) när det skjuts upp i rymden år 2018.
Visar 71 publikationer
JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
A rich hydrocarbon chemistry and high C to O ratio in the inner disk around a very low-mass star
The Mid-infrared Instrument for JWST and Its In-flight Performance
MINDS. The Detection of 13CO
JOYS: Disentangling the warm and cold material in the high-mass IRAS 23385+6053 cluster
Water in the terrestrial planet-forming zone of the PDS 70 disk
Outflows from the youngest stars are mostly molecular
Wavelength calibration and resolving power of the JWST MIRI Medium Resolution Spectrometer
ALMA spectrum of the extreme OH/IR star OH 26.5+0.6
On the nature and mass loss of Bulge OH/IR stars
A chemical survey of exoplanets with ARIEL
On the detection of CO and mass-loss of bulge OH/IR stars
Probing the Dusty Stellar Populations of the Local Volume Galaxies with JWST/MIRI
Mass loss from an extreme OH/IR star: OH 26.5+0.6
The MIRI Medium Resolution Spectrometer calibration pipeline
The ALMA detection of CO rotational line emission in AGB stars in the Large Magellanic Cloud
Herschel/HIFI observations of the circumstellar ammonia lines in IRC+10216
On the Nature of the Enigmatic Object IRAS 19312+1950: A Rare Phase of Massive Star Formation?
Sulphur molecules in the circumstellar envelopes of M-type AGB stars
The Mid-Infrared Instrument for the James Webb Space Telescope, I: Introduction
ALMA observations of α Centauri. First detection of main-sequence stars at 3 mm wavelength
ALMA reveals sunburn: CO dissociation around AGB stars in the globular cluster 47 Tucanae
The Mid-Infrared Instrument for the James Webb Space Telescope, II: Design and Build
H2O Isotopologues in Extreme OH/IR Stars
Classifying the secondary component of the binary star W Aquilae
Detailed Modelling of the Circumstellar Envelope of the S-type AGB Star W Aquilae
The Mid-Infrared Instrument for the James Webb Space Telescope, III: MIRIM, The MIRI Imager
The wind of W Hydrae as seen by Herschel II. The molecular envelope of W Hydrae
Detailed modelling of the circumstellar molecular line emission of the S-type AGB star W Aquilae
The wind of W Hydrae as seen by Herschel I. The CO envelope
OH/IR stars and their superwinds as observed by the Herschel Space Observatory
Multi-line detection of O2 toward rho Ophiuchi A
Herschel/HIFI observations of red supergiants and yellow hypergiants I. Molecular inventory
Herschel/HIFI observations of O-rich AGB stars: molecular inventory
A HIFI View of Circumstellar H2O Emission from the S-type AGB Star X Cyg
Herschel observations of the Herbig-Haro objects HH52-54
The throughput and sensitivity of the JWST mid-infrared instrument
870 µm observations of evolved stars with LABOCA
Polarisation observations of VY Canis Majoris H2O 532-441 620.701 GHz maser emission with HIFI
O(18)O and C(18)O observations of rho Ophiuchi A
Herschel/HIFI deepens the circumstellar NH3 enigma
Discovery of water vapour in the carbon star V Cygni from observations with Herschel/HIFI
Herschel/HIFI observations of high-J CO transitions in the protoplanetary nebula CRL 618
Oxygen in dense interstellar gas : the oxygen abundance of the star forming core ρ Ophiuchi A
Probing the Mass-Loss History of VY CMa
Mapping the PAHs and H2 in ρ Oph A
Modelling of Circumstellar H2O Line Emission from M-type AGB Stars
Recent astroomy highlights from the Odin satellite
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Visar 3 forskningsprojekt
From the beginning to the end of planetary systems: their birth, life and death