HI in the Galaxy
JM Dickey, FJ Lockman - IN: Annual review of astronomy and …, 1990 - adsabs.harvard.edu
An observational review on HI in the Galaxy is presented. Attention is given to observations
of interstellar atomic hydrogen from Lyman-alpha and the 21-cm line through indirect tracers …
of interstellar atomic hydrogen from Lyman-alpha and the 21-cm line through indirect tracers …
Characteristics of nearby interstellar matter
PC Frisch - Space Science Reviews, 1995 - Springer
There is a warm tenuous partially ionized cloud (T∼ 10 4 K, n (HI)∼ 0.1 cm− 3, n (H ii∼
0.22–0.44 cm− 3) surrounding the solar system which regulates the environment of the solar …
0.22–0.44 cm− 3) surrounding the solar system which regulates the environment of the solar …
3D map** of the dense interstellar gas around the Local Bubble
R Lallement, BY Welsh, JL Vergely, F Crifo… - Astronomy & …, 2003 - aanda.org
We present intermediate results from a long-term program of map** the neutral absorption
characteristics of the local interstellar medium, motivated by the availability of accurate and …
characteristics of the local interstellar medium, motivated by the availability of accurate and …
Distances and metallicities of high-and intermediate-velocity clouds
BP Wakker - The Astrophysical Journal Supplement Series, 2001 - iopscience.iop.org
ABSTRACT A table is presented that summarizes published absorption line measurements
for the high-and intermediate-velocity clouds (HVCs and IVCs). New values are derived for …
for the high-and intermediate-velocity clouds (HVCs and IVCs). New values are derived for …
Keck absorption-line spectroscopy of galactic winds in ultraluminous infrared galaxies
In this paper, we present moderately high resolution (~ 65 km s-1) spectroscopy, acquired
with the Echellette Spectrograph and Imager on Keck II, of 11 ultraluminous infrared …
with the Echellette Spectrograph and Imager on Keck II, of 11 ultraluminous infrared …
Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti
Context. The formation and evolution of the Galactic bulge and its relationship with the other
Galactic populations is still poorly understood. Aims. To establish the chemical differences …
Galactic populations is still poorly understood. Aims. To establish the chemical differences …
[HTML][HTML] Map** the contours of the Local bubble: preliminary results
DM Sfeir, R Lallement, F Crifo… - … v. 346, p. 785-797 (1999 …, 1999 - adsabs.harvard.edu
Map** the contours of the Local bubble: preliminary results ADS Classic is now deprecated. It
will be completely retired in October 2019. This page will automatically redirect to the new ADS …
will be completely retired in October 2019. This page will automatically redirect to the new ADS …
Abundance Analysis of Stars at Large Radius in the Sextans Dwarf Spheroidal Galaxy
We present the stellar parameters and chemical abundances of 30 elements for five stars
located at large radii (3.5–10.7 times the half-light radius) in the Sextans dwarf spheroidal …
located at large radii (3.5–10.7 times the half-light radius) in the Sextans dwarf spheroidal …
Optical and infrared photometry of the Type IIn SN 1998S: days 11–146
A Fassia, WPS Meikle, WD Vacca… - Monthly Notices of …, 2000 - academic.oup.com
We present contemporaneous optical and infrared (IR) photometric observations of the Type
IIn SN 1998S covering the period between 11 and 146 d after discovery. The IR data …
IIn SN 1998S covering the period between 11 and 146 d after discovery. The IR data …
New Hubble Space Telescope observations of heavy elements in four metal-poor stars
Elements heavier than the iron group are found in nearly all halo stars. A substantial number
of these elements, key to understanding neutron-capture nucleosynthesis mechanisms, can …
of these elements, key to understanding neutron-capture nucleosynthesis mechanisms, can …