The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.
INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE
Abstract
▪ Abstract The Goddard High-Resolution Spectrograph (GHRS) aboard the Hubble Space Telescope (HST) has yielded precision abundance results for a range of interstellar environments, including gas in the local medium, in the warm neutral medium, in cold diffuse clouds, and in distant halo clouds. Through GHRS studies, investigators have determined the abundances of elements such as C, N, O, Mg, Si, S, and Fe in individual interstellar clouds. These studies have provided new information about the composition of interstellar dust grains, the origin of the Galactic high-velocity cloud system, and the processes that transport gas between the disk and the halo. Precision measurements of the interstellar D to H ratio and of the abundances of r- and s-process elements have also provided fiducial reference values for cosmological and stellar evolutionary observations and theoretical models.
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Cites
CRC Handbook of Chemistry and Physics
(2014) · doi:10.1201/b17118 · Cited by 57,706
Cited by
The interstellar environment of our galaxy
Ferrière, K. M. (2001) · Reviews of Modern Physics · doi:10.1103/revmodphys.73.1031 · Cited by 1,019
Highly Ionized High‐Velocity Gas in the Vicinity of the Galaxy
Sembach, K. R., Wakker, B. P., Savage, B. D., Richter, P., Meade, M., Shull, J. M., Jenkins, E. B., Sonneborn, G., & Moos, H. W. (2003) · The Astrophysical Journal Supplement Series · doi:10.1086/346231 · Cited by 479
Self-citationEvidence of strong quasar feedback in the early Universe
Maiolino, R., Gallerani, S., Neri, R., Cicone, C., Ferrara, A., Genzel, R., Lutz, D., Sturm, E., Tacconi, L. J., Walter, F., et al. (2012) · Monthly Notices of the Royal Astronomical Society: Letters · doi:10.1111/j.1745-3933.2012.01303.x · Cited by 441
Planck early results. XXIV. Dust in the diffuse interstellar medium and the Galactic halo
Planck Collaboration, Abergel, A., Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., Baccigalupi, C., Balbi, A., Banday, A. J., et al. (2011) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201116485 · Cited by 229
Probing the Outflowing Multiphase Gas ∼1 kpc below the Galactic Center
Savage, B. D., Kim, T.-S., Fox, A. J., Massa, D., Bordoloi, R., Jenkins, E. B., Lehner, N., Bland-Hawthorn, J., Lockman, F. J., Hernandez, S., et al. (2017) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/aa8f4c · Cited by 28
“In diffuse ISM cloud absorbers, [Fe/H] is found to range from −2.4 to −1.0 dex, with the smaller abundances found in denser disk gas and the larger abundances found in halo clouds (Savage & Sembach 1996).”
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Metadata
- Authors
- Savage, B. D., & Sembach, K. R.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 1996-09
- Volume
- 34
- Issue
- 1
- Pages
- 279-329
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2123924478
- Cited by
- 1,231
- References
- 1
- FWCI
- 3.99
- Type
- journal article
- Language
- en
- Open access
- closed
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- CoChat. (2026). Citation check: INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE. https://app.cochat.ai/papers/10.1146/annurev.astro.34.1.279
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- Savage, B. D., & Sembach, K. R. (1996). INTERSTELLAR ABUNDANCES FROM ABSORPTION-LINE OBSERVATIONS WITH THE HUBBLE SPACE TELESCOPE. Annual Review of Astronomy and Astrophysics. https://doi.org/10.1146/annurev.astro.34.1.279
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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