Search Publications

The Globular Cluster System in the Inner Region of the Giant Elliptical Galaxy NGC 4472
DOI: 10.1086/301438 Bibcode: 2000AJ....120..260L

Lee, Myung Gyoon; Kim, Eunhyeuk

We present a study of globular clusters in the inner region of the giant elliptical galaxy NGC 4472, based on the HST/WFPC2 archive data. We have found about 1560 globular cluster candidates at the galactocentric radius r<4', most of which are located within r=1.1‧. A V-(V-I) diagram of these objects shows a dominant vertical structure obviousl…

2000 The Astronomical Journal
eHST 18
Physical properties of the pulsating hydrogen-deficient star LSS 3184 (BX Cir)
DOI: 10.48550/arXiv.astro-ph/0004124 Bibcode: 2000A&A...358.1001W

Jeffery, C. S.; Woolf, V. M.

We report new determinations of the radius and mass of the pulsating helium-rich, hydrogen-deficient star LSS 3184 (BX Cir) using measurements of radial velocity and angular radius throughout its pulsation cycle. Measurements of radial velocity, and thus changes in stellar radius (Delta R_star ), were made usi…

2000 Astronomy and Astrophysics
eHST 18
The Ionization Source in the Nucleus of M84
DOI: 10.1086/308741 Bibcode: 2000ApJ...534..189B

Nelson, C.; Green, R. F.; Kaiser, M. E. +9 more

We have obtained new Hubble Space Telescope observations of M84, a nearby massive elliptical galaxy whose nucleus contains a ~1.5×109 Msolar dark compact object, which presumably is a supermassive black hole. Our Space Telescope Imaging Spectrograph spectrum provides the first clear detection of emission lines in the blue (e.…

2000 The Astrophysical Journal
ISO eHST 18
The Triple System HR 7272
DOI: 10.1134/1.20374 Bibcode: 2000AstL...26..116T

Udry, S.; Griffin, R. F.; Tokovinin, A. A. +2 more

A combined spectroscopic-interferometric orbit is computed for the primary component of the visual binary star HR 7272 = ADS 12101. The orbital period is 3.55 years; semimajor axis 0.074 arcsec. Radial velocities of both components were determined by correlation techniques; their semi-amplitudes are 6.6 and 8.4 km/s. Because those amplitudes are s…

2000 Astronomy Letters
Hipparcos 18
Comparative abundance analysis of the hot main sequence stars and their progeny in open cluster M 25
Bibcode: 2000A&A...361..189L

Korotin, S. A.; Andrievsky, S. M.; Kovtyukh, V. V. +2 more

Remarkable inconsistencies between elemental abundances in the main sequence stars and their progeny F-G supergiants are discussed. Comparative abundance analysis of the hot main sequence stars, the cepheid U Sgr and two cool supergiants belonging to young open cluster M 25 is performed. The detected disaccord in the abundances of carbon, oxygen a…

2000 Astronomy and Astrophysics
IUE 18
Radial Color Gradient and Main-Sequence Mass Segregation in M30 (NGC 7099)
DOI: 10.1086/301270 Bibcode: 2000AJ....119.1259H

Guhathakurta, Puragra; Howell, Justin H.; Tan, Amy

It has long been known that the post-core-collapse globular cluster M30 (NGC 7099) has a bluer-inward color gradient, and recent work suggests that the central deficiency of bright red giant stars does not fully account for this gradient. This study uses Hubble Space Telescope Wide Field Planetary Camera 2 images in the F439W and F555W bands, alon…

2000 The Astronomical Journal
eHST 18
Galactic Cosmic Ray Observations at Different Heliospheric Latitudes
DOI: 10.1016/S0273-1177(00)00016-8 Bibcode: 2000AdSpR..26..839H

Heber, Bernd; Potgieter, Marius S.

The local interstellar spectra (LIS) of galactic cosmic rays at low energies cannot be determined from measurements made near Earth, because of strong solar modulation processes from the heliospheric boundary to the observer. Computations done in the seventies based on Parker's cosmic ray modulation theory taking into account diffusion, convection…

2000 Advances in Space Research
Ulysses 18
Experimental Study of External Occulters for the Large Angle and Spectrometric Coronagraph 2: LASCO-C2
DOI: 10.1364/AO.39.003955 Bibcode: 2000ApOpt..39.3955B

Lamy, Philippe; Bout, Maurice; Maucherat, André +2 more

2000 Applied Optics
SOHO 18
Lensing properties of 7 damped Lyalpha absorbing galaxy-QSO pairs
DOI: 10.48550/arXiv.astro-ph/0009433 Bibcode: 2000A&A...363..837L

Surdej, J.; Smette, A.; Le Brun, V. +1 more

Le Brun et al. (1997) presented the first identifications of the galaxies giving rise to 7 intermediate redshift damped Lyalpha (DLA) absorption systems. Here, we study the gravitational lensing properties of these foreground galaxies based on their observed optical appearance and on the absence of any secondary lensed quasar image. We consider th…

2000 Astronomy and Astrophysics
eHST 18
Modeling the Photoionized Interface in Blister H II Regions
DOI: 10.1086/308872 Bibcode: 2000ApJ...535..847S

Hester, J. Jeff; Sankrit, Ravi

We present a grid of photoionization models for the emission from photoevaporative interfaces between the ionized gas and molecular cloud in blister H II regions. For the density profiles of the emitting gas in the models, we use a general power-law form calculated for photoionized, photoevaporative flows by Bertoldi. We find that the spatial emis…

2000 The Astrophysical Journal
eHST 18