100,97 €
118,79 €
-15% su kodu: ENG15
Cataclysmic Variables and Low-Mass X-Ray Binaries
Cataclysmic Variables and Low-Mass X-Ray Binaries
100,97
118,79 €
  • Išsiųsime per 10–14 d.d.
Since 1976 a meeting devoted to recent research on cataclysmic variables (CV workshop) has been held annually somewhere in North America. Many of the meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi- zing a meeting in Massachusetts in the middle of winter. Nobody wants their meeting to go down i…
  • Leidėjas:
  • Metai: 2011
  • Puslapiai: 472
  • ISBN-10: 9401088497
  • ISBN-13: 9789401088497
  • Formatas: 17.8 x 25.4 x 2.4 cm, minkšti viršeliai
  • Kalba: Anglų
  • Extra -15 % nuolaida šiai knygai su kodu: ENG15

Cataclysmic Variables and Low-Mass X-Ray Binaries (el. knyga) (skaityta knyga) | knygos.lt

Atsiliepimai

Aprašymas

Since 1976 a meeting devoted to recent research on cataclysmic variables (CV workshop) has been held annually somewhere in North America. Many of the meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi- zing a meeting in Massachusetts in the middle of winter. Nobody wants their meeting to go down in history as the smallest and dullest, and it surely be the coldest. But on occasion, meeting organizers have defied custom and scheduled meetings for less than-trendy places, and gotten away with it (Ur-bana, IL and Rochester, NY must be reckoned as examples of this). Encouraged by the spatial and temporal proximity of the American Astronomical Society meeting (Boston, January 9-12), we thought we might get away with it again, and so came to organize a meeting for January 12-15, 1983, in Cambridge, MA. There was another reason for a meeting at this time and place, we loftily proclaimed in early mailings. No one doubts that the CV's are closely related to the low-mass X-ray binaries (LMXB' s), in which the accreting star is usually, or perhaps always, more compact than a white dwarf. Many of the general characteristics of LMXB's sound pretty familiar to any student of CV's: orbital periods in the range 0.

EXTRA 15 % nuolaida su kodu: ENG15

100,97
118,79 €
Išsiųsime per 10–14 d.d.

Akcija baigiasi už 1d.23:29:03

Nuolaidos kodas galioja perkant nuo 10 €. Nuolaidos nesumuojamos.

Prisijunkite ir už šią prekę
gausite 1,19 Knygų Eurų!?
Įsigykite dovanų kuponą
Daugiau
  • Leidėjas:
  • Metai: 2011
  • Puslapiai: 472
  • ISBN-10: 9401088497
  • ISBN-13: 9789401088497
  • Formatas: 17.8 x 25.4 x 2.4 cm, minkšti viršeliai
  • Kalba: Anglų Anglų

Since 1976 a meeting devoted to recent research on cataclysmic variables (CV workshop) has been held annually somewhere in North America. Many of the meetings have been held - following a custom older than anyone reading this book - in locations with well-known recreational potential (e. g. Santa Cruz, CA; Boulder, CO). We thought hard about this custom while contemplating the possibility of organi- zing a meeting in Massachusetts in the middle of winter. Nobody wants their meeting to go down in history as the smallest and dullest, and it surely be the coldest. But on occasion, meeting organizers have defied custom and scheduled meetings for less than-trendy places, and gotten away with it (Ur-bana, IL and Rochester, NY must be reckoned as examples of this). Encouraged by the spatial and temporal proximity of the American Astronomical Society meeting (Boston, January 9-12), we thought we might get away with it again, and so came to organize a meeting for January 12-15, 1983, in Cambridge, MA. There was another reason for a meeting at this time and place, we loftily proclaimed in early mailings. No one doubts that the CV's are closely related to the low-mass X-ray binaries (LMXB' s), in which the accreting star is usually, or perhaps always, more compact than a white dwarf. Many of the general characteristics of LMXB's sound pretty familiar to any student of CV's: orbital periods in the range 0.

Atsiliepimai

  • Atsiliepimų nėra
0 pirkėjai įvertino šią prekę.
5
0%
4
0%
3
0%
2
0%
1
0%
(rodomas nebus)