標(biāo)題: Titlebook: Galactic and Extragalactic Infrared Spectroscopy; Proceedings of the X M. F. Kessler,J. P. Phillips Conference proceedings 1984 D. Reidel P [打印本頁] 作者: adulation 時間: 2025-3-21 18:59
書目名稱Galactic and Extragalactic Infrared Spectroscopy影響因子(影響力)
書目名稱Galactic and Extragalactic Infrared Spectroscopy影響因子(影響力)學(xué)科排名
書目名稱Galactic and Extragalactic Infrared Spectroscopy網(wǎng)絡(luò)公開度
書目名稱Galactic and Extragalactic Infrared Spectroscopy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Galactic and Extragalactic Infrared Spectroscopy被引頻次
書目名稱Galactic and Extragalactic Infrared Spectroscopy被引頻次學(xué)科排名
書目名稱Galactic and Extragalactic Infrared Spectroscopy年度引用
書目名稱Galactic and Extragalactic Infrared Spectroscopy年度引用學(xué)科排名
書目名稱Galactic and Extragalactic Infrared Spectroscopy讀者反饋
書目名稱Galactic and Extragalactic Infrared Spectroscopy讀者反饋學(xué)科排名
作者: 歹徒 時間: 2025-3-21 22:45 作者: Inoperable 時間: 2025-3-22 01:08
Audrey D. Goddard,Ellen SolomonESA’s Space Science Department, which used to be called ESLAB, provides the study and project scientist for ESA’s scientific satellite programme. Each year this Department organizes an “ESLAB” symposium and it was decided that the 1982 symposium, held in Toledo, should be devoted to Galactic and Extragalactic Infrared Astronomy.作者: echnic 時間: 2025-3-22 08:05
https://doi.org/10.1007/978-1-4612-0371-1We consider atomic processes relevant to the interpretation of infrared measurements, with special emphasis on important, recent developments.作者: CHASE 時間: 2025-3-22 09:33
Jennifer Li,David Greenwood,Mohamad KassemThe difficulties of making astronomical observations in the submillimeter spectrum are described in detail. Receiver technology and atmospheric absorption provide the biggest challenge. Techniques of overcoming these problems are discussed and some initial astronomical results are illustrated.作者: intertwine 時間: 2025-3-22 15:08
Welcome AddressESA’s Space Science Department, which used to be called ESLAB, provides the study and project scientist for ESA’s scientific satellite programme. Each year this Department organizes an “ESLAB” symposium and it was decided that the 1982 symposium, held in Toledo, should be devoted to Galactic and Extragalactic Infrared Astronomy.作者: intertwine 時間: 2025-3-22 17:05 作者: 蜿蜒而流 時間: 2025-3-22 21:39 作者: 玩忽職守 時間: 2025-3-23 04:41 作者: 猛擊 時間: 2025-3-23 08:48 作者: jocular 時間: 2025-3-23 10:46
https://doi.org/10.1007/978-1-4615-8276-2ill not be discussed here, but identifications, which are based on laboratory data, will be given whenever plausible ones exist. There are a very large number of papers in the literature of even such a young field as infrared spectroscopy, and it is impossible to refer to all of the original sources作者: 兵團 時間: 2025-3-23 13:52
Multisonar-Based Autonomous Indoor Mobility,lity and surface mobility are presented, and the implications for interstellar chemistry are briefly explored. Reactions at the surfaces of oxide grains are reviewed, and their contributions to sulphur-bearing molecules, and hydroxides are described. The disintegration of carbon grains in interstell作者: CLAM 時間: 2025-3-23 20:20 作者: 執(zhí) 時間: 2025-3-23 22:51 作者: Kaleidoscope 時間: 2025-3-24 04:22 作者: 羞辱 時間: 2025-3-24 07:59
Advances in Identity Theory and Researcht studies of H II regions (see, for example, review by Wynn-Williams and Becklin 1974) and of the Becklin-Neugebauer source in Orion (Penston, Allen and Hyland 1971) over the next few years generally confirmed the expectation that hydrogen recombination lines were to be found in H II regions but not作者: ingenue 時間: 2025-3-24 14:16
Multiphoton Microscopy in Urologic Surgerystate of ionization and abundance of different chemical constituents is discussed for clouds exhibiting a range of optical depths. There is a preferred choice of spectral features useful for examining different types of gaseous complexes. The prospects for improving our understanding of chemical rea作者: nocturnal 時間: 2025-3-24 17:13
Molecular Imaging Biomarkers and Agents,sumed to condense, there remains no single source one may point to and confidently say “Indeed, that is a protostar, no need to search further” (cf. Wynn-Williams 1982). The problem is that despite the fact that the photometry gives an excellent assessment of the energy generated within, it tells pa作者: Orthodontics 時間: 2025-3-24 22:36 作者: 印第安人 時間: 2025-3-25 00:48
Pradipta Banerji,Sanjay Chikermanee far-infrared rotational lines of CO, OH, NH. and HD, together with a brief description of the analysis and interpretation of the spectra, The “state of the art” in instrument performance and the prospects for improved sensitivity and resolution are also surveyed.作者: Generic-Drug 時間: 2025-3-25 04:58
Wńodzimierz Bielecki,Dariusz Burakis on determination of the density and temperature structure as well as the velocity field in these objects. The presence of large scale temperature gradients is expected when looking towards embedded heating sources; the frequency with which the expected effects are seen in molecular line data give作者: 好忠告人 時間: 2025-3-25 10:34 作者: 溫室 時間: 2025-3-25 12:44
Phoolendra K. Mishra,Kristopher L. Kuhlmanon towards nearby hot stars, the question of molecule formation has accompanied the observational efforts. These early discoveries by Adams, Dunham, Swings, Rosenfeld and McKellar are separated by a gap of 28 years from the radio-discovery of the first polyatomic molecule ( ammonia, NH. ) in interstellar space by Townes and collaborators.作者: BRACE 時間: 2025-3-25 16:15
Pradipta Banerji,Sanjay Chikermanee far-infrared rotational lines of CO, OH, NH. and HD, together with a brief description of the analysis and interpretation of the spectra, The “state of the art” in instrument performance and the prospects for improved sensitivity and resolution are also surveyed.作者: 性上癮 時間: 2025-3-25 22:07 作者: infinite 時間: 2025-3-26 01:09 作者: Affection 時間: 2025-3-26 05:19
Conference proceedings 1984troscopy 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 l作者: FISC 時間: 2025-3-26 09:11
Absorption and Emission Characteristics of Interstellar Duststressed, rather than those expected from more homogeneous components such as silicates, graphite, or amorphous carbon since these have been discussed in considerable detail elsewhere (e.g. Kr?tschmer and Huffman, 1979, Knacke and Kr?tschmer, 1980, Day, 1979, Borghesi et al., 1983 and references the作者: Agronomy 時間: 2025-3-26 16:43 作者: 希望 時間: 2025-3-26 19:50 作者: 云狀 時間: 2025-3-26 21:54 作者: 中和 時間: 2025-3-27 02:57
The Genetic Aspects of Facial Abnormalities,stressed, rather than those expected from more homogeneous components such as silicates, graphite, or amorphous carbon since these have been discussed in considerable detail elsewhere (e.g. Kr?tschmer and Huffman, 1979, Knacke and Kr?tschmer, 1980, Day, 1979, Borghesi et al., 1983 and references the作者: 蔑視 時間: 2025-3-27 08:24 作者: TOXIN 時間: 2025-3-27 12:03 作者: GROWL 時間: 2025-3-27 15:23
Neven Vr?ek,?eljko Dobrovi?,Dragutin KermekMoreover, infrared observations have shown GMCs to be the primary sites of star birth in our galaxy. Indeed, molecular-line observations of these clouds have given us the first detailed glimpses into the physical processes associated with the earliest stages of stellar evolution and perhaps star for作者: 桶去微染 時間: 2025-3-27 17:55 作者: Ccu106 時間: 2025-3-28 01:39
Absorption and Emission Characteristics of Interstellar Dust. Thus, moderate resolution spectroscopy of the interstellar medium offers unique evidence about the molecules in the condensed and gaseous phases and their distribution. It is the purpose of this paper to discuss the spectral properties of the condensed phase. However, in the astrophysical literatu作者: 大暴雨 時間: 2025-3-28 05:52 作者: 極少 時間: 2025-3-28 08:49
Formation of Molecules on Dustlity and surface mobility are presented, and the implications for interstellar chemistry are briefly explored. Reactions at the surfaces of oxide grains are reviewed, and their contributions to sulphur-bearing molecules, and hydroxides are described. The disintegration of carbon grains in interstell作者: 薄膜 時間: 2025-3-28 11:02 作者: 碌碌之人 時間: 2025-3-28 18:15
Observational Constraints on Interstellar Chemistryon towards nearby hot stars, the question of molecule formation has accompanied the observational efforts. These early discoveries by Adams, Dunham, Swings, Rosenfeld and McKellar are separated by a gap of 28 years from the radio-discovery of the first polyatomic molecule ( ammonia, NH. ) in interst作者: botany 時間: 2025-3-28 19:01
Infrared Spectroscopy of Interstellar Shockss and mass outflow from young stellar objects. There are two types of interstellar shocks: In J shocks, gas properties “jump” from their preshock to their postshock values in a shock front with a thickness < one mean free path; radiation is emitted behind the shock front, primarily in the visible an作者: 我就不公正 時間: 2025-3-29 01:14
Infrared Hydrogen Emission Lines from H II Regions and ‘Protostars’t studies of H II regions (see, for example, review by Wynn-Williams and Becklin 1974) and of the Becklin-Neugebauer source in Orion (Penston, Allen and Hyland 1971) over the next few years generally confirmed the expectation that hydrogen recombination lines were to be found in H II regions but not作者: 漸強 時間: 2025-3-29 06:10 作者: 自愛 時間: 2025-3-29 09:16 作者: CIS 時間: 2025-3-29 15:23
Excitation Conditions in Molecular Cloudsphysical conditions and kinematics of the interstellar gas. By using different molecular transitions we have learned to investigate in quite some detail the molecular clouds, from their tenuous outer surroundings to their dense interiors. In effect molecular transitions are now being used to investi作者: Bricklayer 時間: 2025-3-29 17:24 作者: ACRID 時間: 2025-3-29 21:51
Submillimeter Observations of Molecules and the Structure of Giant Molecular Cloudsis on determination of the density and temperature structure as well as the velocity field in these objects. The presence of large scale temperature gradients is expected when looking towards embedded heating sources; the frequency with which the expected effects are seen in molecular line data give作者: Genome 時間: 2025-3-30 00:07 作者: 確定無疑 時間: 2025-3-30 07:30
Conference proceedings 1984ontribute 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 u作者: epicardium 時間: 2025-3-30 11:14
0067-0057 e 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 procee作者: 有幫助 時間: 2025-3-30 13:04 作者: MAUVE 時間: 2025-3-30 18:52
Ravi V. Kumar,Richard K. Lyon,Jerald A. Coleore detailed comments — fractionation of carbon isotopes, CH. and shocks, the HNC/HCN ratio, the COH./HCO. ratio, fractionation of deuterium and the electron density of interstellar clouds, and the formation of complex molecules.
