Add to ORKGA computerized analysis of a starburst model is discussed. The model proposes that the absorption line equivalent width should scale with the level of star forming activity. Archival International Ultraviolet Explorer (IUE) data on IUE spectra of luminous blue galaxies were compared with previous IUE observations of extragalactic HII regions and low luminosity galaxies. The comparisons are summarized and causes for offsets are discussed
We briefly review, at a level appropriate for graduate students and non-specialists, the field of qu...
We present Keck near-infrared and WIYN (Wisconsin-Indiana-Yale NOAO) optical photometry of a sample ...
We use Keck HIRES spectra of 37 optically bright quasars at z = 2-4 to study narrow absorption lines...
The gas producing the absorption lines seen in the spectra of some high-redshift QSOs can be physica...
We list and analyze H I absorption lines at redshifts 2 = 15 cm(-2). Unlike most prior studies, we u...
We have performed hydrodynamical simulations to investigate the effects of galactic winds on the hig...
The starburst phenomenon was viewed as increasingly important since the recognition that some galaxi...
We study H I and metal-line absorption around z ≈ 2 star-forming galaxies by comparing an analysis o...
We employ detailed photoionization models to infer the physical conditions of intrinsic narrow absor...
The title of this article could of course encompass an entire meeting. I will focus my comments on r...
Researchers are engaged in a multifaceted program to investigate the stellar content and star format...
We study H I and metal-line absorption around z ≈ 2 star-forming galaxies by comparing an analysis o...
During the past five decades astronomers have been puzzled by the presence of strong absorption feat...
Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled ...
We present evidence that clumps of \lya lines are physically associated with about half of the exten...
We briefly review, at a level appropriate for graduate students and non-specialists, the field of qu...
We present Keck near-infrared and WIYN (Wisconsin-Indiana-Yale NOAO) optical photometry of a sample ...
We use Keck HIRES spectra of 37 optically bright quasars at z = 2-4 to study narrow absorption lines...
The gas producing the absorption lines seen in the spectra of some high-redshift QSOs can be physica...
We list and analyze H I absorption lines at redshifts 2 = 15 cm(-2). Unlike most prior studies, we u...
We have performed hydrodynamical simulations to investigate the effects of galactic winds on the hig...
The starburst phenomenon was viewed as increasingly important since the recognition that some galaxi...
We study H I and metal-line absorption around z ≈ 2 star-forming galaxies by comparing an analysis o...
We employ detailed photoionization models to infer the physical conditions of intrinsic narrow absor...
The title of this article could of course encompass an entire meeting. I will focus my comments on r...
Researchers are engaged in a multifaceted program to investigate the stellar content and star format...
We study H I and metal-line absorption around z ≈ 2 star-forming galaxies by comparing an analysis o...
During the past five decades astronomers have been puzzled by the presence of strong absorption feat...
Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled ...
We present evidence that clumps of \lya lines are physically associated with about half of the exten...
We briefly review, at a level appropriate for graduate students and non-specialists, the field of qu...
We present Keck near-infrared and WIYN (Wisconsin-Indiana-Yale NOAO) optical photometry of a sample ...
We use Keck HIRES spectra of 37 optically bright quasars at z = 2-4 to study narrow absorption lines...