Results 91 to 100 of about 21,871 (195)

Diffuse Interstellar Bands: Past and Present [PDF]

Proceedings of the International Astronomical Union, 2013
AbstractThe diffuse interstellar bands (DIBs) have come to the fore as an important mystery. This paper presents the history of DIB discovery and research; their importance; a summary of their properties; constraints on proposed identifications; a survey of DIB papers (including graduate student's theses); and a web site that lists DIBs paper from 1922
openaire   +1 more source

Przezroczystość Wszechświata i międzygwiazdowe pasma rozmyte jako wyzwania dla rozwoju wiedzy przyrodniczej

Zagadnienia Filozoficzne w Nauce, 2017
In general introduction few examples of astronomical explanations of well-known and common local physical phenomena are presented. They are meant to show that it is often much easier to explain commonly experienced phenomena by investigating the behavior
Bogdan Wszołek
doaj  

A search for diffuse bands in fullerene planetary nebulae: evidence of diffuse circumstellar bands

, 2014
Large fullerenes and fullerene-based molecules have been proposed as carriers of diffuse interstellar bands (DIBs). The recent detection of the most common fullerenes (C60 and C70) around some planetary nebulae (PNe) now enable us to study the DIBs ...
Cataldo, F., Diaz-Luis, J. J., Garcia-Hernandez, D. A., Manchado, A., Rao, N. Kameswara   +4 more
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Diffuse interstellar bands in the lab [PDF]

Science, 2015
Astrochemistry The diffuse interstellar bands (DIBs) are a set of hundreds of broad optical/near-infrared absorption features seen throughout the interstellar medium. Despite the first DIBs being discovered as long ago as 1922, none of the bands has ever been convincingly identified with a particular chemical species. Now Campbell et al.
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A search for diffuse bands in the circumstellar envelopes of post-AGB stars

, 2007
In this work we present the results of a systematic search for diffuse bands (DBs, hereafter) in the circumstellar envelopes of a carefully selected sample of post-AGB stars.
Allamandola, Arellano, Arkhipova, Bakker, Bujarrabal, Clube, Cohen, Cox, Cox, Crawford, D. A. García Hernández, de Jong, Desmurs, Douglas, Drimmel, Ehrenfreund, Ehrenfreund, Fernie, Fernández de Córdoba, Fitzgerald, Foing, Fujii, Fulara, Galazutdinov, García-Lario, García-Lario, García-Lario, Gauba, Gauba, Gauba, Guarinos, Guarinos, Heap, Heger, Herbig, Herbig, Hrivnak, Hrivnak, Hrivnak, Hrivnak, Hrivnak, Hrivnak, Hrivnak, Hu, Hu, Iglesias-Groth, Iglesias-Groth, Jenniskens, Kendall, Kerr, Klochkova, Klochkova, Klochkova, Krelowski, Krelowski, Krelowski, Kwok, Kwok, Le Bertre, Le Bertre, Le Bertre, Leger, Lewis, M. A. Satorre, Maas, Malfait, Mauron, McCall, Megier, Meixner, Merrill, N. L. J. Cox, O. Suárez, Oudmaijer, P. García Lario, Parthasarathy, Pottasch, Prichet, R. Luna, Reddy, Reddy, Reed, Reyniers, Ruiterkamp, Salama, Salama, Sarre, Sarre, Scarrott, Snow, Snow, Suárez, te Lintel Hekkert, Thorburn, Torres-Peimbert, Turner, Van de Steene, Van der Veen, Van der Zwet, Van Winckel, Van Winckel, Volk, Weselak, Zacs, Zacs, Zacs, Zacs   +106 more
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Where Have All the Sulfur Atoms Gone? Polycyclic Aromatic Hydrocarbon as a Possible Sink for the Missing Sulfur in the Interstellar Medium. I. The C–S Band Strengths

The Astrophysical Journal
Despite its biogenic and astrochemical importance, sulfur (S), the 10th most abundant element in the interstellar medium (ISM) with a total abundance of S/H ≈ 2.2 × 10 ^−5 , largely remains undetected in molecular clouds.
X. J. Yang, Lijun Hua, Aigen Li
doaj   +1 more source

The Multiwavelength Extinction Law and Its Variation in the Coalsack Molecular Cloud Based on the Gaia, APASS, SMSS, 2MASS, GLIMPSE, and WISE Surveys

The Astrophysical Journal
Accurate interpretation of observations relies on the interstellar dust extinction law, which also serves as a powerful diagnostic for probing dust properties.
Juan Deng, Shu Wang, Biwei Jiang, He Zhao   +3 more
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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 2; peer review: 2 approved]

Open Research Europe
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is ...
Pamela Klaassen, Maria Beltrán, Alessio Traficante, Mark Booth, Kate Pattle, Jonathan Marshall, Joshua Lovell, Brandt Gaches, Alvaro Hacar, Nicolas Peretto, Caroline Bot, Doris Arzoumanian, Thomas Stanke, Gaspard Duchêne, Ana Duarte Cabral, Antonio Hales, David Eden, Patricia Luppe, Jens Kauffmann, Elena Redaelli, Sebastian Marino, Álvaro Sánchez-Monge, Andrew Rigby, Dmitry Semenov, Eugenio Schisano, Mark Thompson, Silvia Spezzano, Claudia Cicone, Friedrich Wyrowski, Martin Cordiner, Tony Mroczkowski, Doug Johnstone, Luca Di Mascolo, Minju Lee, Eelco van Kampen, Thomas Maccarone, Daizhong Liu, Matthew Smith, Amélie Saintonge, Sven Wedemeyer, Alexander Thelen   +40 more
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Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Our Galaxy [version 1; peer review: 2 approved]

Open Research Europe
As we learn more about the multi-scale interstellar medium (ISM) of our Galaxy, we develop a greater understanding for the complex relationships between the large-scale diffuse gas and dust in Giant Molecular Clouds (GMCs), how it moves, how it is ...
Pamela Klaassen, Maria Beltrán, Alessio Traficante, Mark Booth, Kate Pattle, Jonathan Marshall, Joshua Lovell, Brandt Gaches, Alvaro Hacar, Nicolas Peretto, Caroline Bot, Doris Arzoumanian, Thomas Stanke, Gaspard Duchêne, Ana Duarte Cabral, Antonio Hales, David Eden, Patricia Luppe, Jens Kauffmann, Elena Redaelli, Sebastian Marino, Álvaro Sánchez-Monge, Andrew Rigby, Dmitry Semenov, Eugenio Schisano, Mark Thompson, Silvia Spezzano, Claudia Cicone, Friedrich Wyrowski, Martin Cordiner, Tony Mroczkowski, Doug Johnstone, Luca Di Mascolo, Minju Lee, Eelco van Kampen, Thomas Maccarone, Daizhong Liu, Matthew Smith, Amélie Saintonge, Sven Wedemeyer, Alexander Thelen   +40 more
doaj   +1 more source

Are aromatic hydrocarbons the carriers of the diffuse interstellar bands in the visible? [PDF]

Large Polycyclic Aromatic Hydrocarbons (PAH) are the likely origin of the Unidentified Infrared Emission Feature. The molecules or their ions are also attractive candidates for the carriers of the Diffuse Interstellar Bands (DIBs) in the visible range ...
Dhendecourt, L., Leger, A.
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