The Interstellar Medium in Galaxies (Astrophysics and Space Science Library)

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9781402003790: The Interstellar Medium in Galaxies (Astrophysics and Space Science Library)

It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc­ ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen­ tal developments over the past decade: large CCD's became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an "outside" view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way.

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van der Hulst, J.M.
Editorial: Springer 2001-11 (2001)
ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Springer 2001-11, 2001. Estado de conservación: New. This item is printed on demand. Brand new book, sourced directly from publisher. Dispatch time is 24-48 hours from our warehouse. Book will be sent in robust, secure packaging to ensure it reaches you securely. Nº de ref. de la librería NU-LSI-06869913

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Editorial: Kluwer Academic Publishers, United States (2001)
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Descripción Kluwer Academic Publishers, United States, 2001. Paperback. Estado de conservación: New. Language: English . Brand New Book ***** Print on Demand *****.It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc- ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen- tal developments over the past decade: large CCD s became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an outside view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way. Softcover reprint of the original 1st ed. 1997. Nº de ref. de la librería AAV9781402003790

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Editorial: Kluwer Academic Publishers, United States (2001)
ISBN 10: 140200379X ISBN 13: 9781402003790
Nuevos Paperback Cantidad: 10
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The Book Depository US
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Descripción Kluwer Academic Publishers, United States, 2001. Paperback. Estado de conservación: New. Language: English . Brand New Book ***** Print on Demand *****. It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc- ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen- tal developments over the past decade: large CCD s became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an outside view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way. Softcover reprint of the original 1st ed. 1997. Nº de ref. de la librería AAV9781402003790

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ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Estado de conservación: New. This item is Print on Demand - Depending on your location, this item may ship from the US or UK. Nº de ref. de la librería POD_9781402003790

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J.M. van der Hulst
Editorial: Kluwer Academic Publishers (2001)
ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Kluwer Academic Publishers, 2001. 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-9781402003790

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van der Hulst, J.M.
Editorial: Springer (2016)
ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Springer, 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 ria9781402003790_lsuk

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J.M. van der Hulst
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Descripción Kluwer Academic Publishers, 2001. 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-9781402003790

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J.M. VAN DER HULST
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Herb Tandree Philosophy Books
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Descripción Springer, 2001. Paperback. Estado de conservación: NEW. 9781402003790 This listing is a new book, a title currently in-print which we order directly and immediately from the publisher. Nº de ref. de la librería HTANDREE0411914

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Editorial: Kluwer Academic Publishers, United States (2001)
ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Kluwer Academic Publishers, United States, 2001. Paperback. Estado de conservación: New. Language: English . This book usually ship within 10-15 business days and we will endeavor to dispatch orders quicker than this where possible. Brand New Book. It has been more than five decades ago that Henk van de Hulst predicted the observability of the 21-cm line of neutral hydrogen (HI ). Since then use of the 21-cm line has greatly improved our knowledge in many fields and has been used for galactic structure studies, studies of the interstellar medium (ISM) in the Milky Way and other galaxies, studies of the mass distribution of the Milky Way and other galaxies, studies of spiral struc- ture, studies of high velocity gas in the Milky Way and other galaxies, for measuring distances using the Tully-Fisher relation etc. Regarding studies of the ISM, there have been a number of instrumen- tal developments over the past decade: large CCD s became available on optical telescopes, radio synthesis offered sensitive imaging capabilities, not only in the classical 21-cm HI line but also in the mm-transitions of CO and other molecules, and X-ray imaging capabilities became available to measure the hot component of the ISM. These developments meant that Milky Way was no longer the exclusive playground for ISM studies and that by reaching out to other galaxies astronomy had gained the advantage of having an outside view, though at the expense of giving up some linear resolution. Studies of the ISM in other galaxies are intimately connected to studies of the ISM in the Milky Way. Softcover reprint of the original 1st ed. 1997. Nº de ref. de la librería LIE9781402003790

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Editorial: Springer (2013)
ISBN 10: 140200379X ISBN 13: 9781402003790
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Descripción Springer, 2013. Estado de conservación: New. This item is printed on demand for shipment within 3 working days. Nº de ref. de la librería LP9781402003790

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