Search Results - "Lester, Dan F"
-
1
CoolSpec: A Near‐Infrared Long‐Slit Spectrometer for McDonald Observatory
Published in Publications of the Astronomical Society of the Pacific (01-03-2000)“…This paper describes the design, operational goals, and some science accomplishments of the CoolSpec near‐infrared spectrometer on the McDonald Observatory 2.7…”
Get full text
Journal Article -
2
Measuring Stellar Kinematics in Galaxies with the Near-Infrared (2-0) ¹²CO Absorption Bandhead
Published in Publications of the Astronomical Society of the Pacific (01-01-1995)“…The shape and strength of the near-infrared (2-0) ¹²CO absorption bandhead provide astronomers with a unique tool for measuring stellar kinematics in galaxies…”
Get full text
Journal Article -
3
Measuring stellar kinematics in galaxies with the near-infrared (2-0) (12) CO absorption bandhead
Published in Publications of the Astronomical Society of the Pacific (01-01-1995)“…The shape and strength of the near-infrared (2-0) (12)CO absorption bandhead provide astronomers with a unique tool for measuring stellar kinematics in…”
Get full text
Journal Article -
4
Measuring stellar kinematics in galaxies with the near-infrared (2-0) (C-12)O absorption bandhead
Published in Publications of the Astronomical Society of the Pacific (01-01-1995)“…The shape and strength of the near-infrared (2-0) (C-12)O absorption bandhead provide astronomers with a unique tool for measuring stellar kinematics in…”
Get full text
Journal Article -
5
Laboratory studies of the newly discovered infrared band at 4705.2 cm-1 (2.1253 micrometers) in the spectrum of Io: the tentative identification of CO2
Published in Icarus (New York, N.Y. 1962) (1991)“…We discuss over 120 laboratory experiments pertaining to the identification of the new absorption band discovered by Trafton et al. (1991) at 4705.2 cm-1…”
Get more information
Journal Article -
6
The Structure of IR Luminous Galaxies at 100 Microns
Published 29-03-2000“…Astrophys.J.Suppl. 131 (2000) 413-440 We have observed twenty two galaxies at 100 microns with the Kuiper Airborne Observatory in order to determine the size…”
Get full text
Journal Article