Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Kenneth M. Lanzetta"'
Autor:
Michael M. Shara, Kenneth M. Lanzetta, Alexandra Masegian, James T. Garland, Stefan Gromoll, Joanna Mikolajewska, Mikita Misiura, David Valls-Gabaud, Frederick M. Walter, John K. Webb
Publikováno v:
The Astrophysical Journal Letters, Vol 977, Iss 2, p L48 (2024)
A century or less separates the thermonuclear-powered eruptions of recurrent novae (RNe) in the hydrogen-rich envelopes of massive white dwarfs. The colliding ejecta of successive RN events are predicted to always generate very large (tens of parsecs
Externí odkaz:
https://doaj.org/article/70bfc2b1931c49a2b317e9fd3c5de6d0
Autor:
Kenneth M. Lanzetta, Stefan Gromoll, Michael M. Shara, Stephen Berg, David Valls-Gabaud, Frederick M. Walter, John K. Webb
Publikováno v:
Publications of the Astronomical Society of the Pacific. 135:015002
The “Condor Array Telescope” or “Condor” is a high-performance “array telescope” comprised of six apochromatic refracting telescopes of objective diameter 180 mm, each equipped with a large-format, very low-read-noise (≈1.2 e−), very
Autor:
Kenneth M. Lanzetta, Hsiao-Wen Chen
Publikováno v:
The Astrophysical Journal. 597:706-729
We study the nature of damped Lya absorption (DLA) systems at z= -17) to the total neutral gas cross section is not necessary; (4) of the 11 DLAs studied, 45% are disk dominated, 22% are bulge dominated, 11% are irregular, and 22% are in galaxy group
Autor:
Alberto Fernández-Soto, Warrick J. Couch, Paul Bristow, Rogier A. Windhorst, Simon P. Driver, Stephen C. Odewahn, Steven Phillipps, Kenneth M. Lanzetta
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 319:807-812
We combine magnitude and photometric redshift data on galaxies in the Hubble Deep Fields with morphological classifications in order to separate out the distributions for early type galaxies. The updated morphological galaxy number counts down to I =
Publikováno v:
The Astrophysical Journal. 560:101-109
We present an analysis of galaxy and QSO absorption line pairs toward 24 QSOs at redshifts between z~0.2 and 1 in an effort to establish the relationship between galaxies and absorption lines in physical proximity to QSOs. We demonstrate the existenc
Autor:
James E. J. Lovell, B. G. Piner, Smita Mathur, George Chartas, Martin Elvis, Mark Birkinshaw, Belinda Jane Wilkes, Herman L. Marshall, Kajal K. Ghosh, Shanil N. Virani, Robert A. Preston, W. H. Tucker, Diana M Worrall, Steven Tingay, E. J. Hooper, Daniel A. Schwartz, Eric D. Feigelson, Kenneth M. Lanzetta, D. L. Jauncey, Hisashi Hirabayashi, D. E. Harris
Publikováno v:
The Astrophysical Journal. 540:L69-L72
The quasar PKS 0637-753, the first celestial X-ray target of the Chandra X-ray Observatory, has revealed asymmetric X-ray structure extending from 3 to 12 arcsec west of the quasar, coincident with the inner portion of the jet previously detected in
Autor:
Milan M. Ćirković, Kenneth M. Lanzetta
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 315:473-478
Recent measurements of the autocorrelation function of the Ly-alpha clouds are analyzed from the point of view of a simple model with strong clustering on the small scales. It is shown that this toy model reproduces fairly well the important linear r
Publikováno v:
The Astrophysical Journal. 533:120-124
The Hubble Deep Field images have provided us with a unique chance to relate statistical properties of high-redshift galaxies to statistical properties of \lya absorption systems. Combining an {\em empirical} measure of the galaxy surface density ver
Publikováno v:
Scopus-Elsevier
We present new GHRS observations of Lyman alpha absorption lines associated with a group of galaxies towards the QSO 1545+2101. We have identified eight distinct Lyman alpha absorption features in the spectrum of QSO 1545+2101 at a mean redshift of z
Publikováno v:
The Astrophysical Journal. 513:34-50
Using the newly available infrared images of the Hubble Deep Field in the J, H, and K bands and an optimal photometric method, we have refined a technique to estimate the redshifts of 1067 galaxies. A detailed comparison of our results with the spect