An infrared view of protostellar shocks: Near-infrared spectroscopy of star forming regions

ISBN 10: 3639338502 / ISBN 13: 9783639338508
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An infrared view of protostellar shocks: Near-infrared spectroscopy of star forming regions. N° de ref. de la librería

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Sinopsis: The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the "classical" long-slit spectroscopy and the "novel" integral field spectroscopy.

Biografía del autor: Luca Calzoletti was born on 12th May 1978 in Rome. He get Master Degree in Physics at ?La Sapienza? University of Rome and PhD in Physics at the University of Cagliari. His research interests are about infrared astronomy and actually he works as Archive Scientist at the ASI Science Data Centre.

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1.

Luca Calzoletti
Editorial: VDM Verlag 2011-07-31 (2011)
ISBN 10: 3639338502 ISBN 13: 9783639338508
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Descripción VDM Verlag 2011-07-31, 2011. paperback. Estado de conservación: New. Nº de ref. de la librería 9783639338508

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Calzoletti, Luca
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Descripción Estado de conservación: New. Publisher/Verlag: VDM Verlag Dr. Müller | Near-infrared spectroscopy of star forming regions | The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the "classical" long-slit spectroscopy and the "novel" integral field spectroscopy. | Format: Paperback | Language/Sprache: english | 218 gr | 220x150x8 mm | 152 pp. Nº de ref. de la librería K9783639338508

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Luca Calzoletti
Editorial: VDM Verlag Aug 2011 (2011)
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Descripción VDM Verlag Aug 2011, 2011. Taschenbuch. Estado de conservación: Neu. 220x150x9 mm. Neuware - The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the 'classical' long-slit spectroscopy and the 'novel' integral field spectroscopy. 152 pp. Englisch. Nº de ref. de la librería 9783639338508

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Luca Calzoletti
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Descripción VDM Verlag Aug 2011, 2011. Taschenbuch. Estado de conservación: Neu. 220x150x9 mm. This item is printed on demand - Print on Demand Neuware - The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the 'classical' long-slit spectroscopy and the 'novel' integral field spectroscopy. 152 pp. Englisch. Nº de ref. de la librería 9783639338508

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Luca Calzoletti
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Descripción VDM Verlag Aug 2011, 2011. Taschenbuch. Estado de conservación: Neu. 220x150x9 mm. Neuware - The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the 'classical' long-slit spectroscopy and the 'novel' integral field spectroscopy. 152 pp. Englisch. Nº de ref. de la librería 9783639338508

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Luca Calzoletti
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Descripción VDM Verlag, 2011. PAP. Estado de conservación: New. New Book. Delivered from our UK warehouse in 3 to 5 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Nº de ref. de la librería LQ-9783639338508

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Calzoletti, Luca
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Descripción VDM Verlag, 2016. Paperback. Estado de conservación: New. PRINT ON DEMAND Book; New; Publication Year 2016; Not Signed; Fast Shipping from the UK. No. book. Nº de ref. de la librería ria9783639338508_lsuk

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Luca Calzoletti
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Descripción VDM Verlag, 2011. PAP. Estado de conservación: New. New Book. Shipped from US within 10 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Nº de ref. de la librería IQ-9783639338508

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Luca Calzoletti
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Descripción VDM Verlag, Germany, 2011. Paperback. Estado de conservación: New. 220 x 150 mm. Language: English . Brand New Book. The early phases of star formation occur in thick and obscured clouds of dust and molecular gas, where the material collapses under the influence of self-gravity, originating protostars. The process of mass accretion on protostars is one of the less known of the whole stellar evolution. The accretion process goes on through circumstellar disc and part of the infalling material is ejected away from the protostar in form of bipolar jets. Jets can be observed more easily with respect to the circumstellar disc and they often represent the only observational target to reveal the presence of their driving source. Protostellar jets interact with the interstellar medium in the form of shock waves which heat the gas that, in turn, cools by emitting atomic, ionic and molecular lines. Through the analysis of the emission lines it is possible to study the physics and the chemestry of the shocked regions and derive the exchange of energy between the protostar and the interstellar medium. This work presents a study of protostellar jets (HH objects) carried out with two different spectroscopic techniques: the classical long-slit spectroscopy and the novel integral field spectroscopy. Nº de ref. de la librería KNV9783639338508

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Calzoletti, Luca
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Descripción VDM Verlag Dr. Müller, 2011. Paperback. Estado de conservación: New. This item is printed on demand. Nº de ref. de la librería INGM9783639338508

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