Galactic and Extragalactic Infrared Spectroscopy: Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | English |
| Veröffentlicht: |
Dordrecht
Springer Netherlands
1984
|
| Schriftenreihe: | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews
108 |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Beschreibung: | The last major conference on infrared astronomy was the IAU Symposium No. 96 in June 1980. Since then, the discipline has continued to mature and to contribute to all branches of astrophysics. One particular area of growth has been in spectroscopic capabilities at all infrared wavelengths. The purpose of the Symposium in Toledo was to review the scientific questions to be addressed via infrared spectroscopy and to provide, in the proceedings, a useful summary of the field. The sensitivity of infrared spectroscopic observations is still generally limited by detector characteristics or by thermal background radiation. However in recent years improvements in detector technology together with developments in spectroscopic instrumentation have made possible both quite detailed spectroscopy of the brighter members of many classes of galactic sources and also begun to open up some infrared spectroscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem likely in the USA (SIRTF); plans for space submillimeter telescopes are firming up. On the ground large telescopes optimized for infrared observations are now in operation at high altitude sites and specialized submillimeter facilities are under construction. The particular advantages of planned, very large telescopes for infrared observations are widely accepted |
| Beschreibung: | 1 Online-Ressource (XII, 476 p) |
| ISBN: | 9789400972513 9789400972537 |
| ISSN: | 0067-0057 |
| DOI: | 10.1007/978-94-009-7251-3 |
Internformat
MARC
| LEADER | 00000nmm a2200000zcb4500 | ||
|---|---|---|---|
| 001 | BV042415349 | ||
| 003 | DE-604 | ||
| 005 | 00000000000000.0 | ||
| 007 | cr|uuu---uuuuu | ||
| 008 | 150316s1984 |||| o||u| ||||||eng d | ||
| 020 | |a 9789400972513 |c Online |9 978-94-009-7251-3 | ||
| 020 | |a 9789400972537 |c Print |9 978-94-009-7253-7 | ||
| 024 | 7 | |a 10.1007/978-94-009-7251-3 |2 doi | |
| 035 | |a (OCoLC)905442467 | ||
| 035 | |a (DE-599)BVBBV042415349 | ||
| 040 | |a DE-604 |b ger |e aacr | ||
| 041 | 0 | |a eng | |
| 049 | |a DE-91 |a DE-83 | ||
| 082 | 0 | |a 520 |2 23 | |
| 084 | |a PHY 000 |2 stub | ||
| 100 | 1 | |a Kessler, M. F. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Galactic and Extragalactic Infrared Spectroscopy |b Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 |c edited by M. F. Kessler, J. P. Phillips |
| 246 | 1 | 3 | |a Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6-8, 1982 |
| 264 | 1 | |a Dordrecht |b Springer Netherlands |c 1984 | |
| 300 | |a 1 Online-Ressource (XII, 476 p) | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b c |2 rdamedia | ||
| 338 | |b cr |2 rdacarrier | ||
| 490 | 0 | |a Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |v 108 |x 0067-0057 | |
| 500 | |a The last major conference on infrared astronomy was the IAU Symposium No. 96 in June 1980. Since then, the discipline has continued to mature and to contribute to all branches of astrophysics. One particular area of growth has been in spectroscopic capabilities at all infrared wavelengths. The purpose of the Symposium in Toledo was to review the scientific questions to be addressed via infrared spectroscopy and to provide, in the proceedings, a useful summary of the field. The sensitivity of infrared spectroscopic observations is still generally limited by detector characteristics or by thermal background radiation. However in recent years improvements in detector technology together with developments in spectroscopic instrumentation have made possible both quite detailed spectroscopy of the brighter members of many classes of galactic sources and also begun to open up some infrared spectroscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem likely in the USA (SIRTF); plans for space submillimeter telescopes are firming up. On the ground large telescopes optimized for infrared observations are now in operation at high altitude sites and specialized submillimeter facilities are under construction. The particular advantages of planned, very large telescopes for infrared observations are widely accepted | ||
| 650 | 4 | |a Physics | |
| 650 | 4 | |a Astronomy, Observations and Techniques | |
| 700 | 1 | |a Phillips, J. P. |e Sonstige |4 oth | |
| 856 | 4 | 0 | |u https://doi.org/10.1007/978-94-009-7251-3 |x Verlag |3 Volltext |
| 912 | |a ZDB-2-PHA |a ZDB-2-BAE | ||
| 940 | 1 | |q ZDB-2-PHA_Archive | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-027850842 | ||
Datensatz im Suchindex
| _version_ | 1804153082301382656 |
|---|---|
| any_adam_object | |
| author | Kessler, M. F. |
| author_facet | Kessler, M. F. |
| author_role | aut |
| author_sort | Kessler, M. F. |
| author_variant | m f k mf mfk |
| building | Verbundindex |
| bvnumber | BV042415349 |
| classification_tum | PHY 000 |
| collection | ZDB-2-PHA ZDB-2-BAE |
| ctrlnum | (OCoLC)905442467 (DE-599)BVBBV042415349 |
| dewey-full | 520 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 520 - Astronomy and allied sciences |
| dewey-raw | 520 |
| dewey-search | 520 |
| dewey-sort | 3520 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| doi_str_mv | 10.1007/978-94-009-7251-3 |
| format | Electronic eBook |
| fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>03227nmm a2200409zcb4500</leader><controlfield tag="001">BV042415349</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">150316s1984 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400972513</subfield><subfield code="c">Online</subfield><subfield code="9">978-94-009-7251-3</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9789400972537</subfield><subfield code="c">Print</subfield><subfield code="9">978-94-009-7253-7</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/978-94-009-7251-3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)905442467</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV042415349</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">aacr</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="049" ind1=" " ind2=" "><subfield code="a">DE-91</subfield><subfield code="a">DE-83</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">520</subfield><subfield code="2">23</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">PHY 000</subfield><subfield code="2">stub</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Kessler, M. F.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Galactic and Extragalactic Infrared Spectroscopy</subfield><subfield code="b">Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982</subfield><subfield code="c">edited by M. F. Kessler, J. P. Phillips</subfield></datafield><datafield tag="246" ind1="1" ind2="3"><subfield code="a">Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6-8, 1982</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Dordrecht</subfield><subfield code="b">Springer Netherlands</subfield><subfield code="c">1984</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource (XII, 476 p)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews</subfield><subfield code="v">108</subfield><subfield code="x">0067-0057</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">The last major conference on infrared astronomy was the IAU Symposium No. 96 in June 1980. Since then, the discipline has continued to mature and to contribute to all branches of astrophysics. One particular area of growth has been in spectroscopic capabilities at all infrared wavelengths. The purpose of the Symposium in Toledo was to review the scientific questions to be addressed via infrared spectroscopy and to provide, in the proceedings, a useful summary of the field. The sensitivity of infrared spectroscopic observations is still generally limited by detector characteristics or by thermal background radiation. However in recent years improvements in detector technology together with developments in spectroscopic instrumentation have made possible both quite detailed spectroscopy of the brighter members of many classes of galactic sources and also begun to open up some infrared spectroscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem likely in the USA (SIRTF); plans for space submillimeter telescopes are firming up. On the ground large telescopes optimized for infrared observations are now in operation at high altitude sites and specialized submillimeter facilities are under construction. The particular advantages of planned, very large telescopes for infrared observations are widely accepted</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Physics</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astronomy, Observations and Techniques</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Phillips, J. P.</subfield><subfield code="e">Sonstige</subfield><subfield code="4">oth</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1007/978-94-009-7251-3</subfield><subfield code="x">Verlag</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-2-PHA</subfield><subfield code="a">ZDB-2-BAE</subfield></datafield><datafield tag="940" ind1="1" ind2=" "><subfield code="q">ZDB-2-PHA_Archive</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-027850842</subfield></datafield></record></collection> |
| id | DE-604.BV042415349 |
| illustrated | Not Illustrated |
| indexdate | 2024-07-10T01:20:57Z |
| institution | BVB |
| isbn | 9789400972513 9789400972537 |
| issn | 0067-0057 |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-027850842 |
| oclc_num | 905442467 |
| open_access_boolean | |
| owner | DE-91 DE-BY-TUM DE-83 |
| owner_facet | DE-91 DE-BY-TUM DE-83 |
| physical | 1 Online-Ressource (XII, 476 p) |
| psigel | ZDB-2-PHA ZDB-2-BAE ZDB-2-PHA_Archive |
| publishDate | 1984 |
| publishDateSearch | 1984 |
| publishDateSort | 1984 |
| publisher | Springer Netherlands |
| record_format | marc |
| series2 | Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews |
| spelling | Kessler, M. F. Verfasser aut Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 edited by M. F. Kessler, J. P. Phillips Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6-8, 1982 Dordrecht Springer Netherlands 1984 1 Online-Ressource (XII, 476 p) txt rdacontent c rdamedia cr rdacarrier Astrophysics and Space Science Library, A Series of Books on the Recent Developments of Space Science and of General Geophysics and Astrophysics Published in Connection with the Journal Space Science Reviews 108 0067-0057 The last major conference on infrared astronomy was the IAU Symposium No. 96 in June 1980. Since then, the discipline has continued to mature and to contribute to all branches of astrophysics. One particular area of growth has been in spectroscopic capabilities at all infrared wavelengths. The purpose of the Symposium in Toledo was to review the scientific questions to be addressed via infrared spectroscopy and to provide, in the proceedings, a useful summary of the field. The sensitivity of infrared spectroscopic observations is still generally limited by detector characteristics or by thermal background radiation. However in recent years improvements in detector technology together with developments in spectroscopic instrumentation have made possible both quite detailed spectroscopy of the brighter members of many classes of galactic sources and also begun to open up some infrared spectroscopy of extragalactic sources. The potential of the field in the next decade or two is clear. The lRAS mission has completed one of the pre-requisites, namely an all-sky photometric survey. Major space missions utilising cryogenic infrared telescopes have been approved in Europe (ISO) and seem likely in the USA (SIRTF); plans for space submillimeter telescopes are firming up. On the ground large telescopes optimized for infrared observations are now in operation at high altitude sites and specialized submillimeter facilities are under construction. The particular advantages of planned, very large telescopes for infrared observations are widely accepted Physics Astronomy, Observations and Techniques Phillips, J. P. Sonstige oth https://doi.org/10.1007/978-94-009-7251-3 Verlag Volltext |
| spellingShingle | Kessler, M. F. Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 Physics Astronomy, Observations and Techniques |
| title | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 |
| title_alt | Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6-8, 1982 |
| title_auth | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 |
| title_exact_search | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 |
| title_full | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 edited by M. F. Kessler, J. P. Phillips |
| title_fullStr | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 edited by M. F. Kessler, J. P. Phillips |
| title_full_unstemmed | Galactic and Extragalactic Infrared Spectroscopy Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 edited by M. F. Kessler, J. P. Phillips |
| title_short | Galactic and Extragalactic Infrared Spectroscopy |
| title_sort | galactic and extragalactic infrared spectroscopy proceedings of the xvith eslab symposium held in toledo spain december 6 8 1982 |
| title_sub | Proceedings of the XVIth ESLAB Symposium, held in Toledo, Spain, December 6–8, 1982 |
| topic | Physics Astronomy, Observations and Techniques |
| topic_facet | Physics Astronomy, Observations and Techniques |
| url | https://doi.org/10.1007/978-94-009-7251-3 |
| work_keys_str_mv | AT kesslermf galacticandextragalacticinfraredspectroscopyproceedingsofthexvitheslabsymposiumheldintoledospaindecember681982 AT phillipsjp galacticandextragalacticinfraredspectroscopyproceedingsofthexvitheslabsymposiumheldintoledospaindecember681982 AT kesslermf proceedingsofthexvitheslabsymposiumheldintoledospaindecember681982 AT phillipsjp proceedingsofthexvitheslabsymposiumheldintoledospaindecember681982 |