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A hyperluminous galaxy at z=2.8 found in a deep submillimetre survey
DOI: 10.1046/j.1365-8711.1998.01677.x Bibcode: 1998MNRAS.298..583I

Kneib, J. -P.; Ivison, R. J.; Smail, Ian +5 more

We present a detailed study of SMM02399-0136, a hyperluminous, active galaxy selected from a submm survey of the distant Universe. This galaxy is the brightest source in the fields of six rich, lensing clusters, with a total area of 0.01deg^2, that we have mapped with a sensitivity of ~2mJybeam^-1 at 850mum. We identify a compact optical counterpa…

1998 Monthly Notices of the Royal Astronomical Society
eHST 379
Distance to M31 with the Hubble Space Telescope and HIPPARCOS Red Clump Stars
DOI: 10.1086/311539 Bibcode: 1998ApJ...503L.131S

Garnavich, P. M.; Stanek, K. Z.

Following the approach by Paczyński & Stanek, we compare the red clump stars with parallaxes known to better than 10% in the Hipparcos catalog with the red clump stars observed in three fields in M31 using the Hubble Space Telescope. There are ~600 and ~6300 such stars in the two data sets, respectively. The local red clump luminosity function…

1998 The Astrophysical Journal
Hipparcos eHST 377
The Definitive Abundance of Interstellar Oxygen
DOI: 10.1086/305128 Bibcode: 1998ApJ...493..222M

Meyer, David M.; Jura, M.; Cardelli, Jason A.

Using the Goddard High Resolution Spectrograph (GHRS) onboard the Hubble Space Telescope, we have obtained high signal-to-noise (S/N) ratio echelle observations of the weak interstellar O I λ1356 absorption toward the stars γ Cas, ɛ Per, δ Ori, ɛ Ori, 15 Mon, τ CMa, and γ Ara. In combination with previous GHRS measurements in six other sight lines…

1998 The Astrophysical Journal
eHST 369
Infrared Observations of Nebular Emission Lines from Galaxies at Z ~= 3
DOI: 10.1086/306431 Bibcode: 1998ApJ...508..539P

Dickinson, Mark; Giavalisco, Mauro; Pettini, Max +3 more

We present the first results from a program of near-infrared spectroscopy aimed at studying the familiar rest-frame optical emission lines from the H II regions of Lyman break galaxies at z ~= 3. By targeting redshifts that bring the lines of interest into gaps between the strong OH sky emission, we have been successful in detecting Balmer and [O …

1998 The Astrophysical Journal
eHST 365
The Distribution of Nearby Stars in Velocity Space Inferred from HIPPARCOS Data
DOI: 10.1086/300364 Bibcode: 1998AJ....115.2384D

Dehnen, Walter

The velocity distribution f(v) of nearby stars is estimated, via a maximum likelihood algorithm, from the positions and tangential velocities of a kinematically unbiased sample of 14,369 stars observed by the Hipparcos satellite. The distribution f shows rich structure in the radial and azimuthal motions, v_R and v_phi, but not in the vertical vel…

1998 The Astronomical Journal
Hipparcos 361
The Sun's total irradiance: Cycles, trends and related climate change uncertainties since 1976
DOI: 10.1029/1998GL900157 Bibcode: 1998GeoRL..25.4377F

Fröhlich, Claus; Lean, Judith

A composite record of the Sun's total irradiance compiled from measurements made by five independent space-based radiometers since 1978 exhibits a prominent 11-year cycle with similar levels during 1986 and 1996, the two most recent minimum epochs of solar activity. This finding contradicts recent assertions of a 0.04% irradiance increase from the…

1998 Geophysical Research Letters
SOHO 359
New models of Jupiter's magnetic field constrained by the Io flux tube footprint
DOI: 10.1029/97JA03726 Bibcode: 1998JGR...10311929C

Connerney, J. E. P.; Satoh, T.; Acuña, M. H. +1 more

Spherical harmonic models of the planetary magnetic field of Jupiter are obtained from in situ magnetic field measurements and remote observations of the position of the foot of the Io flux tube in Jupiter's ionosphere. The Io flux tube (IFT) footprint locates the ionospheric footprint of field lines traced from Io's orbital radial distance in the…

1998 Journal of Geophysical Research
eHST 341
Detailed Mass Map of CL 0024+1654 from Strong Lensing
DOI: 10.1086/311314 Bibcode: 1998ApJ...498L.107T

Tyson, J. Anthony; Kochanski, Greg P.; Dell'Antonio, Ian P.

We construct a high-resolution mass map of the z=0.39 cluster 0024+1654, based on a parametric inversion of the associated gravitational lens. The lens creates eight well-resolved subimages of a background galaxy, seen in deep imaging with the Hubble Space Telescope.1 Excluding mass concentrations centered on visible galaxies, more than 98% of the…

1998 The Astrophysical Journal
eHST 335
Steps toward interstellar silicate mineralogy. IV. The crystalline revolution
Bibcode: 1998A&A...339..904J

Waters, L. B. F. M.; Mutschke, H.; Henning, Th. +3 more

Mid- and far-infrared spectra gained by the Short Wavelength Spectrometer (SWS) of the Infrared Space Observatory (ISO) satellite have provided striking evidence for the presence of crystalline silicates in comets, circumstellar envelopes around young stars and, most of all, evolved stars and planetary nebulae. Since optical properties of astrophy…

1998 Astronomy and Astrophysics
ISO 334
The Age of Globular Clusters in Light of Hipparcos: Resolving the Age Problem?
DOI: 10.1086/305201 Bibcode: 1998ApJ...494...96C

Chaboyer, Brian; Demarque, P.; Kernan, Peter J. +1 more

We review five independent techniques that are used to set the distance scale to globular clusters, including subdwarf main-sequence fitting utilizing the recent Hipparcos parallax catalog. These data together all indicate that globular clusters are farther away than previously believed, implying a reduction in age estimates. We now adopt a best-f…

1998 The Astrophysical Journal
Hipparcos 322