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Precise Source Locations of Recent Gamma Ray Bursts
Bibcode: 1993ICRC....1...77C

Hurley, K. C.; Fishman, G. J.; Kouveliotou, C. +9 more

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 1
Ulysses 0
How robust are the EGRET AGN gamma-ray identifications?
DOI: 10.1007/BF02512048 Bibcode: 1993NCimC..16..655C

Bignami, G. F.; Caraveo, P.; Ciliegi, P.

Several AGNs have been proposed as identifications of gamma-ray sources discovered by CGRO. Using the NED database, the authors show that these AGNs are not the only extragalactic objects within the error boxes of the sources. Therefore, an in-depth study is needed on a case-by-case basis to access the most probable counterparts of the gamma-ray s…

1993 Nuovo Cimento C Geophysics Space Physics C
COS-B 0
Dependence of Ulysses Low-Energy Proton Flux on Solar Activity
Bibcode: 1993ICRC....3..322A

Anglin, J. D.; Burrows, J. R.; Venkatesan, D. +1 more

1993 23rd International Cosmic Ray Conference (ICRC23), Volume 3
Ulysses 0
Two-component continuum spectrum X-ray pulsar EXO2030+375
DOI: 10.1016/0273-1177(93)90145-2 Bibcode: 1993AdSpR..13l.383S

Li, T. P.; Cheng, L. X.; Sun, X. J. +1 more

We report the detection of a soft X-ray component in the spectrum of the transient X-ray pulsar EXO2030+375 at a high state in 1985. The spectrum of the soft X-ray component could be fitted by a blackbody with a temperature kT ∼1.1 keV and a radius of the emission areaR ∼ 3.6 - 6.1 km (assuming 5 kpc distance).

1993 Advances in Space Research
Exosat 0
HST imaging of the wind-blown lobe NGC 6165.
Bibcode: 1993RMxAA..27..181S

Hester, J.; Scowen, P.; Code, A. +1 more

WFC observations of the lobe NGC 6165 have resolved clumps that are being photoevaporated by the intense UV radiation from HD 148937, in addition to the erosive effects of the strong stellar wind. The central object is a massive superluminous young star that is thought to be undergoing mass loss as it descends onto the main sequence. Analysis of s…

1993 Revista Mexicana de Astronomia y Astrofisica
eHST 0
Ulysses over the pole of the Sun.
Bibcode: 1993AsNow...7...38Y

Young, S.

1993 Astronomy Now
Ulysses 0
The Quality of Photometric Information in the HIPPARCOS Input Catalog
DOI: 10.1086/116612 Bibcode: 1993AJ....105.2344C

Casertano, Stefano; Ratnatunga, Kavan U.; Bell, David J. +1 more

Comparison with independent photoelectric photometry is used to assess the quality of magnitudes and colors in the Hipparcos Input Catalog. These magnitudes and colors will play an important role in the luminosity calibration of Hipparcos stars. We conclude that photoelectric photometry, available for about 37 percent of the catalog, is of uniform…

1993 The Astronomical Journal
Hipparcos 0
Planetary Camera Observations of NGC 1275: Discovery of a Central Population of Compact Massive Blue Star Clusters
DOI: 10.1086/116094 Bibcode: 1992AJ....103..691H

Holtzman, J. A.; Faber, S. M.; Ewald, S. P. +10 more

We have discovered a population of bright blue pointlike sources within 5 kpc of the nucleus of NGC 1275 using HST Planetary Camera observations. The typical object has M_v_ ~ - 12 to - 14 (H_0_ = 75 km s^-1^ Mpc^-1^ ); the brightest has M_v_ ~ - 16. They are all blue, with V - R <~ 0.3. The color distribution and lack of excess Hα emission are…

1992 The Astronomical Journal
eHST 442
The ULYSSES solar wind plasma experiment
Bibcode: 1992A&AS...92..237B

McComas, D. J.; Goldstein, B. E.; Bame, S. J. +5 more

The scientific objectives of the Ulysses solar wind plasma experiment, termed the Solar Wind Observations Over the Poles of the Sun (SWOOPS) include measurements of the solar-wind global properties, the nonlinear MHD disturbances in the solar wind, the internal state of the solar wind plasma, and the solar-wind interaction with Jupiter's magnetic …

1992 Astronomy and Astrophysics Supplement Series
Ulysses 437
Intrinsic parameters of galactic luminous OB stars.
Bibcode: 1992A&A...261..209H

Butler, K.; Kudritzki, R. P.; Herrero, A. +3 more

We present the results of a spectroscopic analysis of 25 galactic luminous OB stars. The gravities are in general lower than previously assumed, especially for giants. The helium abundances are also higher than normal in many cases. Using data from the spectroscopic analysis, radii, luminosities and masses are derived. The observed wind terminal v…

1992 Astronomy and Astrophysics
IUE 434