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Artículos de revistas sobre el tema "Far Ultraviolet Spectroscopic Explorer"

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Publicado: 26 de julio de 2024
Última modificación: 31 de julio de 2025

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1

Moos, Warren. "Lyman the far Ultraviolet Spectroscopic Explorer." International Astronomical Union Colloquium 123 (1990): 171–76. http://dx.doi.org/10.1017/s0252921100077009.

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AbstractThe Lyman Far Ultraviolet Spectroscopic Explorer mission will obtain high resolution spectra (R 30,000) in the 912–1200 Å region with sufficient sensitivity to study faint sources throughout the galaxy and at large extragalactic distances. This spectral region provides unique tools for solving problems in cosmology (e.g. deuterium), galactic structure and evolution (e.g. O VI and H2), stellar evolution (e.g. O VI) and planetary science (e.g. H2). Recent advances in optical and detector technology, which make this goal possible with a moderate size experimental package, also enable the
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2

Moos, Warren. "The Lyman far ultraviolet spectroscopic explorer." Advances in Space Research 11, no. 11 (1991): 221–27. http://dx.doi.org/10.1016/0273-1177(91)90079-y.

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3

Feldman, Paul D. "Spectroscopy of Comets with the Far Ultraviolet Spectroscopic Explorer Satellite." Physica Scripta T119 (January 1, 2005): 7–12. http://dx.doi.org/10.1088/0031-8949/2005/t119/001.

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4

Young, P. R., A. K. Dupree, B. E. Wood, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Capella." Astrophysical Journal 555, no. 2 (2001): L121—L124. http://dx.doi.org/10.1086/322863.

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5

Sonneborn, G., H. W. Moos, and K. R. Sembach. "In-Orbit Performance of the Far Ultraviolet Spectroscopic Explorer." Symposium - International Astronomical Union 198 (2000): 244–46. http://dx.doi.org/10.1017/s0074180900166677.

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The Far Ultraviolet Spectroscopic Explorer (FUSE) satellite was launched by a Delta II rocket on 24 June 1999 into a ˜768 km, 25° orbit. Following the In-Orbit Checkout phase, FUSE is obtaining high-resoluti on spectra (λ/Δλ ≳ 20,000) in the spectral range 905 −1187 Å. The sensitivity meets or exceeds the pre-launch predictions. Many QSOs and AGNs have already been observed.
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6

Murthy, Jayant, and David J. Sahnow. "Observations of the Diffuse Far‐Ultraviolet Background with theFar Ultraviolet Spectroscopic Explorer." Astrophysical Journal 615, no. 1 (2004): 315–22. http://dx.doi.org/10.1086/424441.

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7

Blair, William P., Parviz Ghavamian, Ravi Sankrit, and Charles W. Danforth. "Far Ultraviolet Spectroscopic Explorer Survey of Magellanic Cloud Supernova Remnants." Astrophysical Journal Supplement Series 165, no. 2 (2006): 480–511. http://dx.doi.org/10.1086/505346.

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8

Moos, H. W., W. C. Cash, L. L. Cowie, et al. "Overview of the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Mission." Astrophysical Journal 538, no. 1 (2000): L1—L6. http://dx.doi.org/10.1086/312795.

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9

Hutchings, J. B., A. W. Fullerton, A. P. Cowley та P. C. Schmidtke. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] 900–1200 Å Spectroscopy of AM Herculis". Astronomical Journal 123, № 5 (2002): 2841–46. http://dx.doi.org/10.1086/340080.

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10

Murphy, E. M., K. R. Sembach, B. K. Gibson, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectroscopy of High-Velocity Cloud Complex C." Astrophysical Journal 538, no. 1 (2000): L35—L38. http://dx.doi.org/10.1086/312801.

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11

Sankrit, R., W. P. Blair, and Fuse Snr Team. "Far-ultraviolet Emission from Supernova Remnant Shocks." Symposium - International Astronomical Union 195 (2000): 425–26. http://dx.doi.org/10.1017/s0074180900163399.

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Supernova remnant shocks produce a rich spectrum of lines in the ultraviolet. Among these are important diagnostic resonance lines of O VI, C III, and N III which lie in the bandpass observable with the recently launched Far Ultraviolet Spectroscopic Explorer. We present an overview of a PI program to observe several supernova remnants using this new telescope.
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12

Martin, C., and J. Steiner. "Far–Ultraviolet Background Studies with the Pan–American Astrophysics Explorer (PAX)." Symposium - International Astronomical Union 139 (1990): 456–58. http://dx.doi.org/10.1017/s0074180900241272.

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We describe a proposed far-ultraviolet (FUV) photometric and spectroscopic survey covering the 1300–2000 Å band with a sensitivity comparable to that of the Palomar Sky Survey. Among the numerous scientific objectives of this mission, many have direct bearing on the nature of the FUV background.
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13

Smith, Graeme H. "A Comparison of Publication Counts for Four Ultraviolet Explorer Observatories." Research Notes of the AAS 8, no. 12 (2024): 322. https://doi.org/10.3847/2515-5172/ada156.

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Abstract Publication counts for four space-based ultraviolet observatories are compared: International Ultraviolet Explorer (IUE), Extreme Ultraviolet Explorer, Far Ultraviolet Spectroscopic Explorer (FUSE), and Galaxy Evolution Explorer (GALEX). The first three show rapid rises to either a sharp or broad maximum. Over the peak period for IUE the papers tend to be concentrated upon data from that mission specifically. Maxima are followed by declines of various duration, after which papers based upon multiple space-based observatories have lead to extended relevancy for each mission, particular
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14

Godon, Patrick, Edward M. Sion, Paul E. Barrett, and Paula Szkody. "A FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER SURVEY OF HIGH-DECLINATION DWARF NOVAE." Astrophysical Journal 701, no. 2 (2009): 1091–115. http://dx.doi.org/10.1088/0004-637x/701/2/1091.

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15

Froning, Cynthia S., Knox S. Long, Boris Gänsicke, and Paula Szkody. "A SURVEY OF FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER OBSERVATIONS OF CATACLYSMIC VARIABLES." Astrophysical Journal Supplement Series 199, no. 1 (2012): 7. http://dx.doi.org/10.1088/0067-0049/199/1/7.

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16

Monier, Richard. "The Behavior of HgMn Stars in the Far-UV—Paper 26: HD 207857." Research Notes of the AAS 7, no. 1 (2023): 14. http://dx.doi.org/10.3847/2515-5172/acb54d.

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Abstract The analysis of two spectra of the Mn P Ga spectroscopic binary HD 207857 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of variation of the far-ultraviolet flux of this star over a time interval of about 10 months. The orbital period of this spectroscopic binary being 338.2 days, the observed increases of flux below 1800 Å could be due to the presence of a hot companion.
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17

Dixon, W. Van Dyke, Shauna Sallmen, Mark Hurwitz, and Richard Lieu. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Limits on Far-Ultraviolet Emission from Warm Gas in Clusters of Galaxies." Astrophysical Journal 550, no. 1 (2001): L25—L29. http://dx.doi.org/10.1086/319485.

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18

Sonneborn, George. "Far-Ultraviolet Spectra of Planetary Nebulae." Symposium - International Astronomical Union 209 (2003): 405–11. http://dx.doi.org/10.1017/s0074180900209224.

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The Far Ultraviolet Spectroscopic Explorer (FUSE)> satellite provides a unique opportunity to obtain high-resolution far-UV spectra of a wide variety of astronomical objects, including planetary nebulae. Most FUSE observations of PNe to date have concentrated on the hot central star, providing a very effective way to study the atmosphere of the central star, the surrounding nebula through the absorption features from circumstellar gas. FUSE has found evidence of hot molecular hydrogen in several planetary nebulae, including M27 and BD+30° 3639. Central star spectra also reveal new informati
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19

Duban, Michel. "Comparison of grating designs for the Lyman Far-Ultraviolet Spectroscopic Explorer spectrograph." Applied Optics 32, no. 22 (1993): 4253. http://dx.doi.org/10.1364/ao.32.004253.

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20

Walborn, Nolan R., Alex W. Fullerton, Paul A. Crowther, et al. "Far Ultraviolet Spectroscopic Explorer Atlas of OB Stars in the Magellanic Clouds." Astrophysical Journal Supplement Series 141, no. 2 (2002): 443–68. http://dx.doi.org/10.1086/340571.

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21

Shull, J. Michael, Jason Tumlinson, Edward B. Jenkins, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Diffuse Interstellar Molecular Hydrogen." Astrophysical Journal 538, no. 1 (2000): L73—L76. http://dx.doi.org/10.1086/312782.

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22

Sahnow, D. J., H. W. Moos, T. B. Ake, et al. "On-Orbit Performance of the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Satellite." Astrophysical Journal 538, no. 1 (2000): L7—L11. http://dx.doi.org/10.1086/312794.

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23

Feldman, Paul D., David J. Sahnow, Jeffrey W. Kruk, Edward M. Murphy, and H. Warren Moos. "High-resolution FUV spectroscopy of the terrestrial day airglow with the Far Ultraviolet Spectroscopic Explorer." Journal of Geophysical Research: Space Physics 106, A5 (2001): 8119–29. http://dx.doi.org/10.1029/2000ja000356.

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24

Iping, Rosina, and George Sonneborn. "FUSE Observations of Mass Loss in Planetary Nebulae." Symposium - International Astronomical Union 209 (2003): 187–88. http://dx.doi.org/10.1017/s0074180900208462.

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25

Blair, William P., Ravi Sankrit, and Sean Tulin. "Far Ultraviolet Spectroscopic Explorer and Hopkins Ultraviolet Telescope Observations of Radiative Shocks in the Cygnus Loop." Astrophysical Journal Supplement Series 140, no. 2 (2002): 367–88. http://dx.doi.org/10.1086/342488.

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26

Gruendl, Robert A., You-Hua Chu, and Martín A. Guerrero. "Far Ultraviolet Spectroscopic Explorer Observations of Nebular O vi Emission from NGC 6543." Astrophysical Journal 617, no. 2 (2004): L127—L130. http://dx.doi.org/10.1086/427389.

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27

Danforth, Charles W., J. Christopher Howk, Alex W. Fullerton, William P. Blair, and Kenneth R. Sembach. "An Atlas of Far Ultraviolet Spectroscopic Explorer Sight Lines toward the Magellanic Clouds." Astrophysical Journal Supplement Series 139, no. 1 (2002): 81–189. http://dx.doi.org/10.1086/338239.

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28

Pellerin, Anne, Alex W. Fullerton, Carmelle Robert, et al. "An Atlas of Galactic OB Spectra Observed with the Far Ultraviolet Spectroscopic Explorer." Astrophysical Journal Supplement Series 143, no. 1 (2002): 159–200. http://dx.doi.org/10.1086/342268.

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29

Godon, Patrick, Edward M. Sion, Karen Levay, et al. "AN ONLINE CATALOG OF CATACLYSMIC VARIABLE SPECTRA FROM THE FAR-ULTRAVIOLET SPECTROSCOPIC EXPLORER." Astrophysical Journal Supplement Series 203, no. 2 (2012): 29. http://dx.doi.org/10.1088/0067-0049/203/2/29.

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30

Moos, H. Warren. "FUSE and the Quest for High-Resolution Spectroscopy in the Far Ultraviolet." Highlights of Astronomy 13 (2005): 793–95. http://dx.doi.org/10.1017/s1539299600017147.

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AbstractThe Far Ultraviolet Spectroscopic Explorer (FUSE) instrument covers the spectral range 912-1187 Å with a resolving power of 15,000 to 20,000. This spectral region provides unique access for the study of many atomic and ionic species found in the interstellar medium, intergalactic medium, stars, and extragalactic objects. This paper summarizes the status of the mission and then discusses the need for higher resolution spectroscopy. Although the FUSE instrumental resolution is sufficient to separate most species, it usually it is not adequate for analyzing the gas velocity structure in d
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31

Smith, Graeme H., and Laura E. Langland-Shula. "FUSE Spectroscopy of Two Luminosity Class II Giants." Research Notes of the AAS 7, no. 5 (2023): 98. http://dx.doi.org/10.3847/2515-5172/acd6e9.

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Abstract Analyses have been made of O vi λ1032 and C iii λ977 line profiles in Far Ultraviolet Spectroscopic Explorer spectra of the luminosity class II giants HD 57623 and HD 160635. No conclusive evidence for an outflowing wind could be discerned.
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32

Sonneborn, George, and H. Warren Moos. "First Results from the FUSE Mission." Highlights of Astronomy 12 (2002): 545–91. http://dx.doi.org/10.1017/s1539299600014313.

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AbstractThe Far Ultraviolet Spectroscopic Explorer (FUSE) provides high-resolution spectroscopy at far ultraviolet (FUV) wavelengths (905–1187Å) of many astronomical objects in order to address fundamental questions related to the origin of the universe. FUSE, a cooperative project of the United States, Canada, and France, was launched in June 1999 for a three-year primary mission. The instrument sensitivity permits studies of many extragalactic sources at high spectral resolution. The key science drivers for the mission design are absorption-line spectroscopy of the ISM and IGM to investigate
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33

Shull, J. Michael, Charles W. Danforth, and Katherine L. Anderson. "A Far Ultraviolet Spectroscopic Explorer Survey of Interstellar Molecular Hydrogen in the Galactic Disk." Astrophysical Journal 911, no. 1 (2021): 55. http://dx.doi.org/10.3847/1538-4357/abe707.

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34

Ake, T. B., A. K. Dupree, P. R. Young, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of the Active Cool Star AB Doradus." Astrophysical Journal 538, no. 1 (2000): L87—L90. http://dx.doi.org/10.1086/312796.

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35

Ferlet, R., M. André, G. Hébrard, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of the HD Molecule toward HD 73882." Astrophysical Journal 538, no. 1 (2000): L69—L72. http://dx.doi.org/10.1086/312799.

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36

Good, S. A., M. A. Barstow, M. R. Burleigh, P. D. Dobbie, and J. B. Holberg. "A search for binarity using Far-Ultraviolet Spectroscopic Explorer observations of DAO white dwarfs." Monthly Notices of the Royal Astronomical Society 364, no. 3 (2005): 1082–90. http://dx.doi.org/10.1111/j.1365-2966.2005.09647.x.

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37

Monier, Richard. "The Behavior of HgMn Stars in the Far UV—Paper 27: HD 1909." Research Notes of the AAS 7, no. 1 (2023): 16. http://dx.doi.org/10.3847/2515-5172/acb547.

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Abstract The analysis of two spectra of the spectroscopic binary B9 Hg star HD 1909 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of variations of the far-ultraviolet flux of this star from 1300 up to 2000 Å. The first TESS lightcurve of HD 1909 on the MAST website is periodic with a period close to 7 days which is very close to an earlier period found for the variations of the Strömgren index u. The FUV variations, which occur over about 5 yr, could be caused by the motion of the lower mass companion.
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38

Kim, Jin-Ah, Haeun Chung, Carlos J. Vargas, and Erika Hamden. "UV Cooling via O VI Emission in the Superwind of M82 Observed with the Far Ultraviolet Spectroscopic Explorer (FUSE)." Astronomical Journal 168, no. 1 (2024): 11. http://dx.doi.org/10.3847/1538-3881/ad4887.

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Abstract We examined archival Far Ultraviolet Spectroscopic Explorer data to search for far-ultraviolet emission lines in the starburst galaxy M82. The observations were made in an outflow region that extends beyond the galactic disk. We found the O vi λ λ 1032, 1038 emission lines from the galaxy’s southern outflow region. The O vi lines suggest that the outflowing warm-hot gas is undergoing radiative cooling. We measured a radial velocity of ∼420 km s−1 from the O vi lines, which is faster than the velocity seen in Hα observations. The O vi λ1038 emission line seems to be blended with the C
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39

Welsh, B. Y., D. M. Sfeir, S. Sallmen, and R. Lallement. "Far Ultraviolet Spectroscopic Explorer observations of high-velocity gas associated with the Monoceros Loop SNR." Astronomy & Astrophysics 372, no. 2 (2001): 516–26. http://dx.doi.org/10.1051/0004-6361:20010502.

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40

Mallouris, Christoforos. "The Complete Far Ultraviolet Spectroscopic Explorer Spectrum of the Small Magellanic Cloud Star Sk 108." Astrophysical Journal Supplement Series 147, no. 2 (2003): 265–303. http://dx.doi.org/10.1086/375339.

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41

Wakker, B. P., B. D. Savage, K. R. Sembach, et al. "The Far Ultraviolet Spectroscopic Explorer Survey of O vi Absorption in and near the Galaxy." Astrophysical Journal Supplement Series 146, no. 1 (2003): 1–123. http://dx.doi.org/10.1086/346230.

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42

Rachford, Brian L., Theodore P. Snow, Joshua D. Destree, et al. "MOLECULAR HYDROGEN IN THE FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER TRANSLUCENT LINES OF SIGHT: THE FULL SAMPLE." Astrophysical Journal Supplement Series 180, no. 1 (2008): 125–37. http://dx.doi.org/10.1088/0067-0049/180/1/125.

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43

Chambord, Sylvain, Robert Grange, Jean Flamand, Michel Saïsse, and Jean-Louis Reynaud. "Holographic gratings for the Far Ultraviolet Spectroscopic Explorer: development, imaging, and efficiency tests of two prototypes." Applied Optics 35, no. 19 (1996): 3653. http://dx.doi.org/10.1364/ao.35.003653.

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44

Sembach, K. R., B. D. Savage, J. M. Shull, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of O [CSC]vi[/CSC] in High-Velocity Clouds." Astrophysical Journal 538, no. 1 (2000): L31—L34. http://dx.doi.org/10.1086/312785.

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45

Oegerle, W. R., T. M. Tripp, K. R. Sembach, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of the Galactic and Intergalactic Medium toward H1821+643." Astrophysical Journal 538, no. 1 (2000): L23—L26. http://dx.doi.org/10.1086/312798.

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46

Hoard, D. W., Paula Szkody, Ryoko Ishioka, et al. "Observations of the Magnetic Cataclysmic Variable VV Puppis with the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL]." Astronomical Journal 124, no. 4 (2002): 2238–44. http://dx.doi.org/10.1086/342547.

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47

Sterling, N. C., Harriet L. Dinerstein, and Charles W. Bowers. "Discovery of Enhanced Germanium Abundances in Planetary Nebulae with the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL]." Astrophysical Journal 578, no. 1 (2002): L55—L58. http://dx.doi.org/10.1086/344473.

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48

Kriss, G. A. "Resolving the Structure of Ionized Helium in the Intergalactic Medium with the Far Ultraviolet Spectroscopic Explorer." Science 293, no. 5532 (2001): 1112–16. http://dx.doi.org/10.1126/science.1062693.

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49

Crowther, Paul A., A. W. Fullerton, D. J. Hillier, et al. "[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectroscopy of the O [CSC]vi[/CSC] Resonance Doublet in Sand 2 (WO)." Astrophysical Journal 538, no. 1 (2000): L51—L55. http://dx.doi.org/10.1086/312783.

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50

Monier, Richard. "The Behavior of HgMn Stars in the Far UV—Paper 25: HD 77350." Research Notes of the AAS 7, no. 1 (2023): 11. http://dx.doi.org/10.3847/2515-5172/acb34c.

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Abstract The analysis of five spectra of the Hg Mn spectroscopic binary star HD 77350 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of variation of the far-ultraviolet flux of this star shortwards of 1800 Å. The analysis of the coadded SWP spectrum built from the high resolution SWP spectra obtained through the small aperture shows the importance of low excitation and resonance Si ii lines shortwards of 1540 Å, of the Ga ii and Ga iii resonance lines at 1414 and 1495 Å and of the Al ii resonance line at 1670 Å. A very rough estimate of a period
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