Web Analytics Made Easy - StatCounter
Catalogue of Stellar Ultraviolet Fluxes Nandy K and GI Thompson

Catalogue of Stellar Ultraviolet Fluxes Nandy K and GI Thompson

<

Catalogue of Stellar Ultraviolet Fluxes Nandy K. and G.I. Thompson:

1, but for t And, an F8 V star.

Continuum-normalized spectrum of HD 215227 from the first and second nights (the latter

Fig. 1.

Model fitted to observed photometric fluxes for HD 26367. The four filled circles in the

Photometry of PM.

GALEX FUV and NUV around Stars

Fig. 22.

α Arae (unresolved star + uniform disc) model diameters (in mas) dependence

00003_psisdg9604_960403_page_18_1.jpg

00003_psisdg9604_960403_page_10_2.jpg

Albedos estimated in the ISM of the MW. (a) The diffuse Galactic light

Fig. 9.

Fig. 2.

Observation Log

E (B-V) determination from an UV-visual two-colour diagram: O and B stars in the catalogue of stellar ultraviolet fluxes

Differences of dust models. The panel (a) shows the extinction laws (extinction

00003_psisdg9604_960403_page_16_1.jpg

Fig. 17.

HD 144277 in the HR-diagram: post-main sequence evolutionary tracks (solid

Catalogue of Stellar Ultraviolet Fluxes: A compilation: Thompson, G.I.; K.

Fig. 5.

Compact Sources { NGC 1079 .

α Arae (unresolved star + uniform disc) model upper limit diameters (in mas

00003_psisdg9604_960403_page_17_1.jpg

An illustration of the T eff , [M/H], log g degeneracy

Fig. 15.

Albedos estimated in the interstellar medium of the Milky Way. (a) The diffuse

00003_psisdg9604_960403_page_14_1.jpg

The Aging Brain and Senile Dementia (Advances: Editor-K. Nandy

FUV line luminosities and comparison with the Cygnus Loop and the Vela

... improved observational data for the model fitting, and improved fitting techniques, the largest change in the modeled IR fluxes of Bohlin ...

Accelerator and Radiation Physics: P. K. Sarkar,

Observations of Interstellar Reddening. 2. Results for: Nandy, K.

Physical Parameters for HD 26367

00003_psisdg9604_960403_page_12_1.jpg

HD 26367: A Nearby, Newly Identified Barium Dwarf

Parameters of asteroseismic models of HD 144277 and comparison with the results from spectroscopy.

Figure 2.

Fig. 4.—

IUE Observing Log .

HST images of the nuclear ring in NGC 2997. Left panel: FOC F220W (

Figure 1.

Figure 19.

”Toy” models used in order to fit the AMBER and MIDI measurements. The. ”

Figure 8.

Standard image ...

Scatter plot of the FUV intensity against dust extinction: the blue, orange, and

FUV Line Luminosities and Comparisons with the Cygnus Loop

Observed fluxes and excesses of δ Vel compared to the Castelli & Kurucz (2003 .

where

Distance of the Scattering Layer from the Star

Flatness ratio of the projected envelope versus opening angle calculted with our simple disc model for

00003_psisdg9604_960403_page_15_1.jpg

Figure 30.

DSO spectrum of HD 26367 (middle) compared with the F8 III MK standard Peg

The computed flux from 92 to 560 nm (dashed) compared

HR 7409 (7 Vul)

Figure 4.

Figure 2.

Figure 16.

Fig. 3.

Fluxes of the FIMS, TD1-F1565, and SKYLAB compared with those of the

00003_psisdg9604_960403_page_10_1.jpg

Fig. 11.

Figure 6.

Figure 12.

Figure 15.

Contours of C IV (λ ∼ 1550Å1550Å) emission intensity are displayed over an Hα

Figure 13.

00003_psisdg9604_960403_page_11_2.jpg

Fig. 1.—

Figure 2.

On the nature of the Be star HR 7409 (7 Vul)

Fig. 14.

Fig. 13.

A compilation of fluxes derived from magnitudes reported in the literature. Uncertainties are quoted .

The SPEAR L-channel spectra. Spectra of regions XA+NE cloud, Carrot

The Nature of Unidentified Galactic High-Energy Gamma-Ray Sources

Fig. 3.—

Fig. 6.

Continued

Figure 7.

00003_psisdg9604_960403_page_13_2.jpg

Figure 22.

Standard image ...

Figure 15.

Figure 5.

Radial velocity (Hα core)

Figure 3.

Histogram of the number of sources versus the measured Faust magnitudes.

Figure 18.

Figure 14.

Dependence of the ultraviolet excess on the lithium content in late giants

The FAUST image of the Ophiuchus field. The elon- gated stellar images are the

Figure 6.

Figure 2.

dentification of Bright Stars Observed with SPEAR

Figure 31.

NTT and KPNO spectra of bright sdB and sdO stars from the GALEX selection ranked according

Catalogue of Stellar Ultraviolet Fluxes Nandy K. and G.I. Thompson:

1, but for t And, an F8 V star.

Model fitted to observed photometric fluxes for HD 26367. The four filled circles in the

Fig. 1.

00003_psisdg9604_960403_page_13_2.jpg

Photometry of PM.

GALEX FUV and NUV around Stars

Fig. 22.

00003_psisdg9604_960403_page_18_1.jpg

Continuum-normalized spectrum of HD 215227 from the first and second nights (the latter

Fig. 2.

00003_psisdg9604_960403_page_10_2.jpg

α Arae (unresolved star + uniform disc) model diameters (in mas) dependence

Albedos estimated in the ISM of the MW. (a) The diffuse Galactic light

Observation Log

Fig. 9.

Albedos estimated in the interstellar medium of the Milky Way. (a) The diffuse

Fig. 17.

Differences of dust models. The panel (a) shows the extinction laws (extinction

00003_psisdg9604_960403_page_16_1.jpg

E (B-V) determination from an UV-visual two-colour diagram: O and B stars in the catalogue of stellar ultraviolet fluxes

HD 144277 in the HR-diagram: post-main sequence evolutionary tracks (solid

Fig. 15.

Compact Sources { NGC 1079 .

Fig. 5.

00003_psisdg9604_960403_page_17_1.jpg

00003_psisdg9604_960403_page_14_1.jpg

Catalogue of Stellar Ultraviolet Fluxes: A compilation: Thompson, G.I.; K.

... improved observational data for the model fitting, and improved fitting techniques, the largest change in the modeled IR fluxes of Bohlin ...

HD 26367: A Nearby, Newly Identified Barium Dwarf

00003_psisdg9604_960403_page_12_1.jpg

α Arae (unresolved star + uniform disc) model upper limit diameters (in mas

The Aging Brain and Senile Dementia (Advances: Editor-K. Nandy

Physical Parameters for HD 26367

Accelerator and Radiation Physics: P. K. Sarkar,

Observations of Interstellar Reddening. 2. Results for: Nandy, K.

FUV line luminosities and comparison with the Cygnus Loop and the Vela

Figure 19.

Figure 2.

Fig. 4.—

Parameters of asteroseismic models of HD 144277 and comparison with the results from spectroscopy.

IUE Observing Log .

Figure 1.

Standard image ...

Fluxes of the FIMS, TD1-F1565, and SKYLAB compared with those of the

Figure 8.

Scatter plot of the FUV intensity against dust extinction: the blue, orange, and

HST images of the nuclear ring in NGC 2997. Left panel: FOC F220W (

FUV Line Luminosities and Comparisons with the Cygnus Loop

Observed fluxes and excesses of δ Vel compared to the Castelli & Kurucz (2003 .

where

Distance of the Scattering Layer from the Star

Flatness ratio of the projected envelope versus opening angle calculted with our simple disc model for

Figure 30.

DSO spectrum of HD 26367 (middle) compared with the F8 III MK standard Peg

00003_psisdg9604_960403_page_15_1.jpg

The computed flux from 92 to 560 nm (dashed) compared

HR 7409 (7 Vul)

Figure 4.

”Toy” models used in order to fit the AMBER and MIDI measurements. The. ”

Figure 16.

Fig. 3.

00003_psisdg9604_960403_page_10_1.jpg

Fig. 11.

Figure 6.

Figure 12.

Figure 15.

Contours of C IV (λ ∼ 1550Å1550Å) emission intensity are displayed over an Hα

Figure 13.

Fig. 1.—

On the nature of the Be star HR 7409 (7 Vul)

Figure 2.

00003_psisdg9604_960403_page_11_2.jpg

Fig. 14.

Fig. 13.

00003_psisdg9604_960403_page_13_1.jpg

A compilation of fluxes derived from magnitudes reported in the literature. Uncertainties are quoted .

The SPEAR L-channel spectra. Spectra of regions XA+NE cloud, Carrot

Fig. 3.—

Fig. 6.

Continued

Figure 7.

Figure 22.

Standard image ...

Radial velocity (Hα core)

Figure 15.

Figure 3.

Histogram of the number of sources versus the measured Faust magnitudes.

Figure 18.

Figure 14.

Dependence of the ultraviolet excess on the lithium content in late giants

The FAUST image of the Ophiuchus field. The elon- gated stellar images are the

Figure 6.

Figure 2.

dentification of Bright Stars Observed with SPEAR

Figure 31.

NTT and KPNO spectra of bright sdB and sdO stars from the GALEX selection ranked according

Figure 10.

00003_psisdg9604_960403_page_12_2.jpg

WFPC2 datasets analyzed in this paper .