Search Publications

Distance to the Virgo cluster galaxy M100 from Hubble Space Telescope observations of Cepheids
DOI: 10.1038/371757a0 Bibcode: 1994Natur.371..757F

Illingworth, Garth D.; Kennicutt, Robert C.; Madore, Barry F. +11 more

Accurate distances to galaxies are critical for determining the present expansion rate of the Universe or Hubble constant (H0). An important step in resolving the current uncertainty in H0 is the measurement of the distance to the Virgo cluster of galaxies. New observations using the Hubble Space Telescope yield a distance of…

1994 Nature
eHST 452
Detection of intergalactic ionized helium absorption in a high-redshift quasar
DOI: 10.1038/370035a0 Bibcode: 1994Natur.370...35J

Boksenberg, A.; Deharveng, J. M.; Jakobsen, P. +3 more

Observations obtained with the recently refurbished Hubble Space Telescope reveal strong absorption arising from singly ionized helium along the line of sight to a high-redshift quasar. The strength of the absorption suggests that it may arise in a diffuse ionized intergalactic medium. The detection also confirms that substantial amounts of helium…

1994 Nature
eHST 220
Evidence for a quasar in the radio galaxy Cygnus A from observation of broad-line emission
DOI: 10.1038/371313a0 Bibcode: 1994Natur.371..313A

Antonucci, Robert; Hurt, Todd; Kinney, Anne

ACTIVE galaxies are thought to be powered by the accretion of surrounding dust and gas onto central black holes. The unified model1-3 of active galaxies predicts that narrow-line radio galaxies (NLRGs), which are very luminous at radio wavelengths and have narrow optical emission lines, would appear as quasars—which have broad emission …

1994 Nature
eHST 69
Dust formation in Nova Cassiopeiae 1993 seen by ultraviolet absorption
DOI: 10.1038/369539a0 Bibcode: 1994Natur.369..539S

Sonneborn, G.; Hauschildt, P. H.; Shore, S. N. +2 more

The clouds of gas in interstellar space also contain grains of dust, whose properties and origins have been the focus of debate for decades. Some dust formation has been assumed to take place in novae explosions1-5, as was first implied by the observation of a steep decrease in the amount of light emitted by the nova1,2 DQ He…

1994 Nature
IUE 48
Discovery of Jovian dust streams and interstellar grains by the Ulysses spacecraft
DOI: 10.1038/362428a0 Bibcode: 1993Natur.362..428G

Forsyth, R.; Balogh, A.; Bame, S. J. +20 more

ON 8 February 1992, the Ulysses spacecraft flew by Jupiter at a distance of 5.4 AU from the Sun. During the encounter, the spacecraft was deflected into a new orbit, inclined at about 80° to the ecliptic plane, which will ultimately lead Ulysses over the polar regions of the Sun1. Within 1 AU from Jupiter, the onboard dust de…

1993 Nature
Ulysses 336
Mechanism for the acceleration and ejection of dust grains from Jupiter's magnetosphere
DOI: 10.1038/363144a0 Bibcode: 1993Natur.363..144H

Horanyi, M.; Grun, E.; Morfill, G.

PERHAPS the most unexpected finding of the Ulysses mission so far has been the detection of quasi-periodic streams of high-velocity, submicrometre-sized dust particles during the spacecraft's encounter with Jupiter1. The impact geometry clearly shows that these small grains originate in the jovian system, but it is surprising that any d…

1993 Nature
Ulysses 242
A large nuclear accretion disk in the active galaxy NGC4261
DOI: 10.1038/364213a0 Bibcode: 1993Natur.364..213J

O'Connell, Robert W.; Ferrarese, Laura; Ford, Holland C. +2 more

THE powerful emissions from the nuclei of active galaxies and quasars are thought to arise from the accretion of matter onto a massive black hole. Angular momentum will prevent matter from falling directly onto the central mass; instead, an 'accretion disk' should form, within which the gravitationally bound material will lose angular momentum and…

1993 Nature
eHST 151
Detection of the hydroxyl radical in the Saturn magnetosphere
DOI: 10.1038/363329a0 Bibcode: 1993Natur.363..329S

Shemansky, D. E.; Tripp, T. M.; Matheson, P. +2 more

THE magnetosphere in the vicinity of the orbits of Saturn's icy satellites consists of a low-density plasma, in which the electrons are an order of magnitude cooler than the accompanying heavy ions1. Most models2-12 neglect this fact, even though radiative cooling and diffusive loss rates are both too slow to account for the …

1993 Nature
eHST 139
Ejection of dust from Jupiter's gossamer ring
DOI: 10.1038/364695a0 Bibcode: 1993Natur.364..695H

Hamilton, Douglas P.; Burns, Joseph A.

ONE of the most intriguing discoveries of the Ulysses mission so far has been the detection of periodic, collimated streams of high-velocity, submicrometre-sized dust particles emanating from Jupiter1,2. To explain the Ulysses data, Horanyi et al. showed3 that electromagnetic forces within Jupiter's magnetosphere can accelera…

1993 Nature
Ulysses 65
Dust particle impacts during the Giotto encounter with comet Grigg-Skjellerup
DOI: 10.1038/362732a0 Bibcode: 1993Natur.362..732M

Colangeli, L.; Green, S. F.; Greenberg, J. M. +7 more

IN the European Space Agency's 1992 Giotto Extended Mission, the Dust Impact Detection System operated successfully during a fly-by that took the spacecraft within about 200 km of the nucleus of comet Grigg-Skjellerup. During the encounter, three meteoroid impacts were detected on Giotto's front shield. The particle masses were found to be lOO

1993 Nature
Giotto 61