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Article
High Resolution WFPC2 Imaging of IRAS 09104 + 4109
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Article
A near infrared speckle imaging study of T Tauri Stars
The results of a speckle imaging survey of T Tauri stars suggest that most, if not all, young low mass stars have companions. Repeated observations of these young binary stars have revealed orbital motion in t...
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Chapter
Photodissociation Regions in Young PN
Infrared imaging of H2 and PAH emission in NGG 7027 and BD+30 3639 reveals the presence of photodissociation regions in the neutral gas surrounding these young planetary nebulae.
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Chapter
Near- and Mid-IR Imaging of the Nuclear Starburst in NGC 3079
The nearly edge-on Sc galaxy NGC 3079 displays strong nuclear optical emission lines of Ha, Hβ, [NII], [SII], [OI] and [OIII], and has been classified as a LINER based on the widths and relative fluxes of these l...
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Chapter
Near-Infrared Imaging of Ultraluminous IRAS Galaxies
IRAS discovered a class of objects which emit most of their radiation at infrared wavelengths and which possess bolometric luminosities comparable to those of classical quasars. Due to their extreme power, and...
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Chapter
A near Infrared Speckle Imaging Study of T Tauri Stars
The results of a speckle imaging survey of T Tauri stars suggest that most, if not all, young low mass stars have companions. Repeated observations of these young binary stars have revealed orbital motion in t...
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Chapter and Conference Paper
Ultraluminous Infrared Galaxies and the Origin of Quasars
The Infrared Astronomical Satellite (IRAS) has discovered a class of ultraluminous infrared galaxies (L ir > 1012 L ⊙) that are bolometrically as luminou...
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Chapter and Conference Paper
Millimeter Observations of Luminous IRAS Galaxies
We have observed a group of luminous IRAS galaxies in the continuum at 1.25mm with the Caltech Submillimeter Observatory in 1988 May and September. Table I lists the galaxies and their measured flux densities ...
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Chapter and Conference Paper
High luminosity galaxies in the IRAS survey
The IRAS survey has demonstrated the existence of a previously unrecognized class of ultraluminous objects. These ultraluminous infrared galaxies represent the dominant population of extragalactic emitters at ...
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Chapter
IRAS Observations of Active Galaxies
The IRAS survey gives an unbiased view of the infrared properties of the active galaxies. Seyfert galaxies occupy much the same area in color-color plots as do normal infrared bright galaxies, but extend the r...
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Chapter and Conference Paper
Bäcklund transformations in general relativity
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Article
Entropy and gravitation
Einstein's gravitational theory is analyzed from a thermodynamic point of view. A thermodynamic potential characterizing the sources of gravitational fields is presented. By means of this potential the entropy...
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Chapter and Conference Paper
High Resolution Map** of the Orion Nebula Region at 30, 50 and 100 Microns
The central ~4’ x 4’ region of the Orion Nebula-OMC1 complex has been mapped with 20” resolution in well-defined bands at 30, 50, and 100 µ from the NASA C-141 infrared observatory. These data provide detailed...
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Chapter and Conference Paper
High resolutions maps of the galactic center at 2.2 and 10 μ
Photometric maps of the central 1' of the Galactic center are presented at 2.2 and 10μ with a spatial resolution of ≈ 2'.'5. Most of the 2.2-μ radiation within the central 2 pc comes from discrete sources with...
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Chapter
New Infrared Sources Associated with H ii Regions
Photometry and map** in the wavelength range 1.65–20μ of the H ii regions W3 and NGC 7538 have led to the discovery of a dozen new infrared emission sources. The sources have flux densities ranging up to 10-23 ...
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Chapter
Mariner 1969: Results of the Infrared Radiometer Experiment
The energy radiated by Mars in the wavelength bands 8–12 and 18–25 μ has been measured during the flyby of Mariner 1969 with linear resolution of 50 km at closest approach. From the laboratory energy calibrations...
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Article
Zu axialsymmetrischen stationären Lösungen der Einsteinschen Feldgleichungen für das Vakuum
For axialsymmetric stationary vacuum fields Einstein equations reduce to a system, derivable from a simple Lagrangian. An investigation of its forminvariance leads to a method to construct from known solutions...
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Article
Algebraisch spezielle Einstein-Räume mit einer Bewegungsgruppe
In algebraically special Einstein spaces (Rμv=0) with a hypersurfaceorthogonal spacelike Killing vector field ξv, the trajectories of the multiple eigen null directions kμ lie — except one case — in the subspaces