Multiwavelength approaches to understanding interstellar dust

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Perhaps more than almost any other subject of astrophysical study, the interstellar medium can be studied at any wavelength-from gamma rays to the radio-with each waveband providing unique and significant information. However, there are substantial limitations on the available data. One such limitation is the fact that very few lines of sight have been adequately observed in multiple wavebands. This in turn restricts our understanding of topics as fundamental as interstellar abundances and dust composition. I will review the reasons that such data limitations exist and specifically describe two accepted observing programs that will, in the near future, utilize a multiwavelength approach in studying interstellar dust. The first is a Chandra/HST program that will provide unique insight into dust composition by disentangling the gas-phase and dust-phase abundances of oxygen and iron. The second is a Spitzer/HST program that will examine the extinction curves of possible "translucent clouds" at wavelengths from the UV to the IR.

Original languageEnglish (US)
Title of host publicationFuture Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission
Pages113-115
Number of pages3
DOIs
StatePublished - Dec 18 2009
EventFuture Directions in Ultraviolet Spectroscopy Conference - Annapolis, MD, United States
Duration: Oct 20 2008Oct 22 2008

Publication series

NameAIP Conference Proceedings
Volume1135
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherFuture Directions in Ultraviolet Spectroscopy Conference
CountryUnited States
CityAnnapolis, MD
Period10/20/0810/22/08

Fingerprint

dust
wavelengths
line of sight
astrophysics
extinction
gamma rays
vapor phases
iron
oxygen
curves

Keywords

  • Dust-abundances
  • ISM:-abundances

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Jensen, A. G. (2009). Multiwavelength approaches to understanding interstellar dust. In Future Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission (pp. 113-115). (AIP Conference Proceedings; Vol. 1135). https://doi.org/10.1063/1.3154028

Multiwavelength approaches to understanding interstellar dust. / Jensen, Adam G.

Future Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. 2009. p. 113-115 (AIP Conference Proceedings; Vol. 1135).

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Jensen, AG 2009, Multiwavelength approaches to understanding interstellar dust. in Future Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. AIP Conference Proceedings, vol. 1135, pp. 113-115, Future Directions in Ultraviolet Spectroscopy Conference, Annapolis, MD, United States, 10/20/08. https://doi.org/10.1063/1.3154028
Jensen AG. Multiwavelength approaches to understanding interstellar dust. In Future Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. 2009. p. 113-115. (AIP Conference Proceedings). https://doi.org/10.1063/1.3154028
Jensen, Adam G. / Multiwavelength approaches to understanding interstellar dust. Future Directions in Ultraviolet Spectroscopy - A Conference Inspired by the Accomplishments of the Far Ultraviolet Spectroscopic Explorer Mission. 2009. pp. 113-115 (AIP Conference Proceedings).
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