ISBN 10: 1581122349 / ISBN 13: 9781581122343
Gebraucht / Anzahl: 0
Bei weiteren Verkäufern erhältlich
Alle  Exemplare dieses Buches anzeigen

Über dieses Buch

Leider ist dieses Exemplar nicht mehr verfügbar. Wir haben Ihnen weitere Exemplare dieses Titels unten aufgelistet.

Beschreibung:

Brand New, Unread Copy in Perfect Condition. A+ Customer Service!. Buchnummer des Verkäufers

Über diesen Titel:

Bewertung (bereitgestellt von Goodreads):
5 durchschnittlich
(2 Bewertungen)

Inhaltsangabe: Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the >1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky.

„Über diesen Titel“ kann sich auf eine andere Ausgabe dieses Titels beziehen.

Bibliografische Details

Zustand: New

Beste Suchergebnisse bei AbeBooks

1.

Kaplan, David L.
Verlag: Dissertation.Com. 2004-07-01 (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Anzahl: 5
Anbieter
Chiron Media
(Wallingford, Vereinigtes Königreich)
Bewertung
[?]

Buchbeschreibung Dissertation.Com. 2004-07-01, 2004. PF. Buchzustand: New. Buchnummer des Verkäufers NU-LSI-06906264

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 21,45
Währung umrechnen

In den Warenkorb

Versand: EUR 3,46
Von Vereinigtes Königreich nach Deutschland
Versandziele, Kosten & Dauer

2.

David L Kaplan
Verlag: Dissertation.com (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Anzahl: > 20
Print-on-Demand
Anbieter
Books2Anywhere
(Fairford, GLOS, Vereinigtes Königreich)
Bewertung
[?]

Buchbeschreibung Dissertation.com, 2004. PAP. Buchzustand: New. New Book. Delivered from our UK warehouse in 3 to 5 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Buchnummer des Verkäufers LQ-9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 22,88
Währung umrechnen

In den Warenkorb

Versand: EUR 11,56
Von Vereinigtes Königreich nach Deutschland
Versandziele, Kosten & Dauer

3.

David L Kaplan
Verlag: DISSERTATION.COM, United States (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 10
Print-on-Demand
Anbieter
The Book Depository US
(London, Vereinigtes Königreich)
Bewertung
[?]

Buchbeschreibung DISSERTATION.COM, United States, 2004. Paperback. Buchzustand: New. 242 x 188 mm. Language: English . Brand New Book ***** Print on Demand *****. Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the >1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky. Buchnummer des Verkäufers AAV9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 26,02
Währung umrechnen

In den Warenkorb

Versand: Gratis
Von Vereinigtes Königreich nach Deutschland
Versandziele, Kosten & Dauer

4.

David L Kaplan
Verlag: DISSERTATION.COM, United States (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 10
Print-on-Demand
Anbieter
The Book Depository
(London, Vereinigtes Königreich)
Bewertung
[?]

Buchbeschreibung DISSERTATION.COM, United States, 2004. Paperback. Buchzustand: New. 242 x 188 mm. Language: English Brand New Book ***** Print on Demand *****.Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the >1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky. Buchnummer des Verkäufers AAV9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 26,04
Währung umrechnen

In den Warenkorb

Versand: Gratis
Von Vereinigtes Königreich nach Deutschland
Versandziele, Kosten & Dauer

5.

David L Kaplan
Verlag: Dissertation.com (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Anzahl: > 20
Print-on-Demand
Anbieter
Pbshop
(Wood Dale, IL, USA)
Bewertung
[?]

Buchbeschreibung Dissertation.com, 2004. PAP. Buchzustand: New. New Book. Shipped from US within 10 to 14 business days. THIS BOOK IS PRINTED ON DEMAND. Established seller since 2000. Buchnummer des Verkäufers IQ-9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 24,42
Währung umrechnen

In den Warenkorb

Versand: EUR 13,35
Von USA nach Deutschland
Versandziele, Kosten & Dauer

6.

Kaplan, David L.
Verlag: Dissertation.Com. (2016)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 1
Print-on-Demand
Anbieter
Ria Christie Collections
(Uxbridge, Vereinigtes Königreich)
Bewertung
[?]

Buchbeschreibung Dissertation.Com., 2016. Paperback. Buchzustand: New. PRINT ON DEMAND Book; New; Publication Year 2016; Not Signed; Fast Shipping from the UK. No. book. Buchnummer des Verkäufers ria9781581122343_lsuk

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 26,86
Währung umrechnen

In den Warenkorb

Versand: EUR 4,79
Von Vereinigtes Königreich nach Deutschland
Versandziele, Kosten & Dauer

7.

Kaplan, David L.
Verlag: Dissertation.Com. (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Softcover Anzahl: 1
Anbieter
European-Media-Service Mannheim
(Mannheim, Deutschland)
Bewertung
[?]

Buchbeschreibung Dissertation.Com., 2004. Buchzustand: New. Buchnummer des Verkäufers GM9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 32,61
Währung umrechnen

In den Warenkorb

Versand: Gratis
Innerhalb Deutschland
Versandziele, Kosten & Dauer

8.

Kaplan, David L.
Verlag: Dissertation.Com. (2017)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 10
Print-on-Demand
Anbieter
Murray Media
(North Miami Beach, FL, USA)
Bewertung
[?]

Buchbeschreibung Dissertation.Com., 2017. Paperback. Buchzustand: New. This item is printed on demand. Buchnummer des Verkäufers 1581122349

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 30,23
Währung umrechnen

In den Warenkorb

Versand: EUR 17,79
Von USA nach Deutschland
Versandziele, Kosten & Dauer

9.

David L. Kaplan
Verlag: Dissertation.Com. (2004)
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 1
Anbieter
Ergodebooks
(RICHMOND, TX, USA)
Bewertung
[?]

Buchbeschreibung Dissertation.Com., 2004. Paperback. Buchzustand: New. Buchnummer des Verkäufers DADAX1581122349

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 35,33
Währung umrechnen

In den Warenkorb

Versand: EUR 12,46
Von USA nach Deutschland
Versandziele, Kosten & Dauer

10.

David L. Kaplan
Verlag: Dissertation.Com.
ISBN 10: 1581122349 ISBN 13: 9781581122343
Neu Paperback Anzahl: 20
Anbieter
BuySomeBooks
(Las Vegas, NV, USA)
Bewertung
[?]

Buchbeschreibung Dissertation.Com. Paperback. Buchzustand: New. Paperback. 284 pages. Dimensions: 9.5in. x 7.4in. x 0.7in.Neutron stars are invaluable tools for exploring stellar death, the physics of ultra-dense matter, and the effects of extremely strong magnetic fields. The observed population of neutron stars is dominated by the 1000 radio pulsars, but there are distinct sub-populations that, while fewer in number, can have significant impact on our understanding of the issues mentioned above. These populations are the nearby, isolated neutron stars discovered by ROSAT, and the central compact objects in supernova remnants. The studies of both of these populations have been greatly accelerated in recent years through observations with the Chandra X-ray Observatory and the XMM-Newton telescope. First, we discuss radio, optical, and X-ray observations of the nearby neutron stars aimed at determining their relation to the Galactic neutron star population and at unraveling their complex physical processes by determining the basic astronomical parameters that define the population---distances, ages, and magnetic fields---the uncertainties in which limit any attempt to derive basic physical parameters for these objects. We conclude that these sources are 1e6 year-old cooling neutron stars with magnetic fields above 1e13 Gauss. Second, we describe the hollow supernova remnant problem: why many of the supernova remnants in the Galaxy have no indication of central neutron stars. We have undertaken an X-ray census of neutron stars in a volume-limited sample of Galactic supernova remnants, and from it conclude that either many supernovae do not produce neutron stars contrary to expectation, or that neutron stars can have a wide range in cooling behavior that makes many sources disappear from the X-ray sky. This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Paperback. Buchnummer des Verkäufers 9781581122343

Weitere Informationen zu diesem Verkäufer | Frage an den Anbieter

Neu kaufen
EUR 38,94
Währung umrechnen

In den Warenkorb

Versand: EUR 11,52
Von USA nach Deutschland
Versandziele, Kosten & Dauer

Es gibt 1 weitere Exemplare dieses Buches

Alle Suchergebnisse ansehen