Author: Edward Singleton Holden
Publisher:
ISBN:
Category : Orion Nebula
Languages : en
Pages : 230
Book Description
Monograph of the Central Parts of the Nebula of Orion (R.A. 5h 28m 24s.O, N.P.D. 95029ʹ10ʺ.9, 1860.0)
Author: Edward Singleton Holden
Publisher:
ISBN:
Category : Orion Nebula
Languages : en
Pages : 230
Book Description
Publisher:
ISBN:
Category : Orion Nebula
Languages : en
Pages : 230
Book Description
MONOGRAPH OF THE CENTRAL PARTS OF THE NEBULA OF ORION
Author: EDWARD SINGLETON. HOLDEN
Publisher:
ISBN: 9781033055830
Category :
Languages : en
Pages : 0
Book Description
Publisher:
ISBN: 9781033055830
Category :
Languages : en
Pages : 0
Book Description
Monograph of the Central Parts of the Nebula of Orion ...
Author: Edward Singleton Holden
Publisher:
ISBN:
Category : Orion (Constellation).
Languages : en
Pages : 260
Book Description
Publisher:
ISBN:
Category : Orion (Constellation).
Languages : en
Pages : 260
Book Description
Monograph of the Central Parts of the Nebula of Orion
Author: Edward S. Holden
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 230
Book Description
The main object of this memoir is to leave such measures and descriptions of the brightest parts of the nebula of Orion as shall enable another person observing in after years with the same telescope, under like conditions, to say with certainty whether no changes have occurred in these parts of the nebula. The brightest parts are chosen so as to avoid as far as possible any uncertainty in the conclusion then to be reached, and also because there is little to be added to the complete observations of Lord Rosse and of G. P. Bond on the fainter portions. A second and an important object is to make a thorough discussion of the vast mass of material now at hand.
Publisher:
ISBN:
Category : Astronomy
Languages : en
Pages : 230
Book Description
The main object of this memoir is to leave such measures and descriptions of the brightest parts of the nebula of Orion as shall enable another person observing in after years with the same telescope, under like conditions, to say with certainty whether no changes have occurred in these parts of the nebula. The brightest parts are chosen so as to avoid as far as possible any uncertainty in the conclusion then to be reached, and also because there is little to be added to the complete observations of Lord Rosse and of G. P. Bond on the fainter portions. A second and an important object is to make a thorough discussion of the vast mass of material now at hand.