10-MU-M AND 20-MU-M SPECTROPOLARIMETRY OF THE BN OBJECT

10-MU-M AND 20-MU-M SPECTROPOLARIMETRY OF THE BN OBJECT

Bibliografiska uppgifter
Huvudupphovsmän:	Aitken, D, Smith, C, Roche, P
Materialtyp:	Journal article
Publicerad:	1989

Liknande verk

THE STRUCTURE OF THE NARROW EMISSION BANDS NEAR 10-MU-M
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THE EMISSION STRUCTURE BETWEEN 11-MU-M AND 13-MU-M ACROSS THE ORION IONIZATION FRONT
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MULTICOLOR, 8-13-MU-M MAPS OF THE CENTRAL PARSEC OF THE GALAXY
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An investigation of the 3-mu m emission bands in planetary nebulae
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SPECTROPOLARIMETRY OF THE 3-MU-M ICE FEATURE IN MOLECULAR CLOUDS .2. GL 2591, GL 2136, W33A AND ELIAS 29 (RHO-OPHIUCHI DARK CLOUD)
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8-13 mu m dust emission features in Galactic bulge planetary nebulae
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MIDINFRARED STUDIES OF ETA-CARINAE .2. POLARIMETRIC IMAGING AT 12.5 MU-M AND THE MAGNETIC-FIELD STRUCTURE
av: Aitken, D, et al.
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MIDINFRARED STUDIES OF ETA-CARINAE .1. SUBARCSECOND IMAGING AT 12.5 AND 17 MU-M
av: Smith, C, et al.
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Spectropolarimetry of the 3 micron ice feature toward the Becklin-Neugebauer object
av: Hough, J, et al.
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MIDINFRARED SPECTROPOLARIMETRY OF MWC 349 - A HYDROMAGNETICALLY DRIVEN OUTFLOW
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Studies in mid-infrared spectropolarimetry - II. An atlas of spectra
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12-mu m fine-structure emission line and continuum images of G333.6-0.2
av: Fujiyoshi, T, et al.
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The emission band at 5.25 mu m and its relationship to the unidentified emission features at 11-13 and 3.4-3.6 mu m
av: Roche, P, et al.
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Spectropolarimetry of the 3 micron ice feature toward the becklin-neugebauer object 1
av: Hough, J, et al.
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INFRARED SPECTROPOLARIMETRY OF AFGL-2591 - EVIDENCE FOR AN ANNEALED GRAIN COMPONENT
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THE NATURE OF DUST GRAINS IN THE CLOUDS OF MAGELLAN - 8-13-MU-M SPECTRA OF LMC N44A AND SMC N88A
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The spatial variation of the 3-mu m dust features in Circinus
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Infrared spectropolarimetry of Seyfert galaxy NGC1068
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STUDIES IN MIDINFRARED SPECTROPOLARIMETRY .1. MAGNETIC-FIELDS, DISKS AND FLOWS IN STAR FORMATION REGIONS
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HerMES: deep number counts at 250 mu m, 350 mu m and 500 mu m in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
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Determination of mass limits around pulsars at 10 and 90 mu m with ISO
av: Miramond, L, et al.
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Observations of relativistic plasma waves excited by a 1.064 mu m and 1.053 mu m laser beat
av: Dyson, A, et al.
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Diaquahexa-mu(2)-dichloroacetato-mu(3)-oxido-tetrahydrofurandiiron(III)m anganese(II)
av: Sadeghi, O., et al.
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THE OXFORD 1-MU-M PROTON MICRO-PROBE
av: Watt, F, et al.
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Lyman break and ultraviolet-selected galaxies at z similar to 1-II. PACS 100 mu m/160 mu m FIR detections
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Search for D+(s) to pi+ mu+ mu- and D+(s) to pi- mu+ mu+ decays
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Search for the rare decays B+-->mu+mu-K+, B-->mu+mu-K*(892), and Bs-->mu+mu- phi at CDF
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Hyperfine splitting of [Al VI] 3.66 mu m and the Al isotopic ratio in NGC 6302
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Supersymmetric large tan(beta) corrections to DeltaM_(d,s) and B_(d,s) -> mu+mu- revisited
av: Freitas, A, et al.
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Low-noise single-photon detection at wavelength 1.55 mu m
av: Hiskett, P, et al.
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Search for B-S(0) -> mu(+)mu(-) and B-0 -> mu(+)mu(-) decays
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Search for the rare decays B-s(0) -> mu(+)mu(-) and B-0 -> mu(+)mu(-)
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The coronal line regions of planetary nebulae NGC 6302 and 6537: 3-13 mu m grating and echelle spectroscopy
av: Casassus, S, et al.
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Search for B-s(0) -> mu(+)mu(-) and B-0 -> mu(+)mu(-) Decays with CDF II
av: Aaltonen, T, et al.
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Strong Constraints on the Rare Decays B-s(0) -> mu(+)mu(-) and B-0 -> mu(+)mu(-)
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Analysis of 1.55[mu]m semiconductor lasers for modelocked operation
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