Cassinelli, Joseph P.
Joseph P. Cassinelli astronome
Cassinelli, Joseph P., 1940-....
VIAF ID: 10018130 (Personal)
Permalink: http://viaf.org/viaf/10018130
Preferred Forms
- 200 _ | ‡a Cassinelli ‡b Joseph P.
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- 100 1 _ ‡a Cassinelli, Joseph P. (sparse)
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- 100 1 0 ‡a Cassinelli, Joseph P.
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- 100 1 _ ‡a Cassinelli, Joseph P. ‡d 1940-...
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- 100 1 _ ‡a Cassinelli, Joseph P., ‡d 1940-....
- 100 0 _ ‡a Joseph P. Cassinelli ‡c astronome
4xx's: Alternate Name Forms (14)
Works
Title | Sources |
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Combined satellite and ground-based observations of the quiescent high latitude symbiotic variable AG Draconis = BD +67 922 | |
Comment on the IRAS infrared spectrum of zeta Puppis (O4 If) | |
Constraints from Infrared Space Observatory data on the velocity law and clumpiness of WR 136 | |
Constraints on the physical properties of optical bullets in SS 433 | |
Early magnetic b-type stars: X-ray emission and wind properties | |
The eddington limit upper boundary for cool stars on the HR diagram | |
The effect of linearly polarized light from extended stellar atmospheres on interferometer response functions | |
The effect of rotational gravity darkening on magnetically torqued Be star discs | |
The Effects of Clumps in Explaining X‐Ray Emission Lines from Hot Stars | |
The effects of winds and coronae of hot stars on the infrared and radio continua | |
Equatorial disk formation around rotating stars due to ram pressure | |
EUVE spectroscopy of epsilon Canis Majoris (B2 II) from 70 to 730 A | |
Evidence for a disk in the wind of HD 93521 : UV line profiles from an axymmetric model | |
Expanding envelopes of early-type stars: current status | |
Extended model atmospheres for the central stars of planetary nebulae | |
An extensive collection of stellar wind X-ray source region emission line parameters, temperatures, velocities, and their radial distributions as obtained from Chandra observations of 17 OB stars | |
Finite source depolarization factors for circumstellar scattering | |
The hanle effect as a diagnostic of magnetic fields in stellar envelopes. I. Theoretical results for integrated line profiles | |
High-resolution X-ray spectra of the brightest OB stars in the Cygnus OB2 association | |
High-resolution X-ray spectroscopy of $\tau$ Scorpii (B0.2V) with XMM-Newton | |
Highly accelerated diamagnetic plasmoids: a new X-ray production mechanism for OB stellar winds | |
Hot star polarimetric variability and the nature of wind inhomogeneities | |
The importance of XUV radiation as a solution to the p V mass loss rate discrepancy in O stars | |
Inference of steady stellar wind v(r) laws from optically thin emission lines. III. Inversion of total line intensity distributions | |
Influence of abundances on mass-loss determination for WC stars | |
An infrared study of three Wolf-Rayet ring nebulae | |
Introduction to stellar winds, 1998: | |
Magnetic fields in massive stars. II. The buoyant rise of magnetic flux tubes through the radiative interior | |
Magnetically fed hot star Keplerian disks with slow outflow | |
Main-sequence B stars with strong winds in the core of NGC 6231 | |
Mass-loss rates for eta Carinae as affected by equatorial wind compression | |
Massive stars, 1993: | |
Massive stars, their lives in the interstellar medium : proceedings of a symposium held as part of the 104th Annual Meeting of the Astronomical Society of the Pacific, at the University of Wisconsin, Madison, Wisconsin, 23-25 June 1992 | |
Modelling X-ray variability in the structured atmospheres of hot stars | |
Neon abundances from a Spitzer/IRS survey of Wolf-Rayet stars | |
New challenges for wind shock models: the Chandra spectrum of the hot star {delta} Orionis | |
On the polarization of alpha Orionis | |
On the surface magnetic fields of rapidly rotating stars with winds | |
Optically thick clumps - not the solution to the Wolf-Rayet wind momentum problem? | |
ORFEUS-SPAS II extreme-ultraviolet spectroscopy of {epsilon} CMa (B2 II) | |
Periodic outbursts in the peculiar X-ray binary 2S 0114+65 | |
Polarization by rotationally distorted electron scattering atmospheres | |
Polarization in massive X-ray binaries. I. A low-inclination model for Cygnus X-1 | |
Polarization models for a two-component wind in early-type stars | |
Polarization variability arising from clumps in the winds of Wolf-Rayet stars | |
Pre-outburst spectra of nova RS Ophiuchi 1967 | |
Predicted extreme-ultraviolet line emission for nearby main-sequence B stars | |
Properties of R 136a as derived from its optical light distribution | |
Properties of the supermassive star R136a | |
Protodiscs around hot magnetic rotator stars | |
Results from an extensive Einstein stellar survey | |
The ROSAT all-sky survey catalogue of optically bright OB-type stars | |
ROSAT and EUVE observations of B stars | |
Search for optical coronal line emission from the X-ray sources epsilon Orionis (B0 IA) and kappa Orionis (B0.5 IA) | |
Shock-generated X-ray emission in radiatively driven winds: a model for tau Scorpii | |
Simultaneous X-ray and ultraviolet observations of Epsilon Orionis and Kappa Orionis | |
The spectral energy distribution of zeta Puppis and HD 50896 | |
Stagnation and Infall of Dense Clumps in the Stellar Wind of τ Scorpii | |
Stellar winds and the EUV continuum excess of early B-giants | |
The structure of the winds and coronae of O stars derived from H alpha line-profile analyses | |
SWS observations of IR emission features towards compact HII regions | |
Terminal speeds and ion fractions from [Ca IV] 3.207 {mu}m in three single WN stars | |
Time-dependent behavior of linear polarization in unresolved photospheres, with applications for the Hanle effect | |
Ultraviolet observations of R136a, the superluminous central object of the 30 Doradus nebula | |
VLA radio continuum measurements of mass loss from early-type stars | |
``WCFields'': a magnetic rotating stellar wind model from wind compression theory | |
Wolf-Rayet wind structure and optical variability | |
XMM-Newton observations of β Centauri (B1 III): The temperature structure in the hot plasma and the photosphere-wind connection | |
XMM-Newton observations of ζ Orionis (O9.7 Ib): a collisional ionization equilibrium model |