A Population of Hot, Dusty Ultraluminous Galaxies atz≈ 2

2004 ◽  
Vol 614 (2) ◽  
pp. 671-678 ◽  
Author(s):  
S. C. Chapman ◽  
Ian Smail ◽  
A. W. Blain ◽  
R. J. Ivison
Keyword(s):  
Ultraluminous Galaxies

scholarly journals Zeeman splitting in OH megamasers

2007 ◽  
Vol 3 (S242) ◽  
pp. 467-470
Author(s):  
Timothy Robishaw ◽  
Carl Heiles ◽  
Eliot Quataert
Keyword(s):  
Emission Line ◽  
Zeeman Effect ◽  
Zeeman Splitting ◽  
Ultraluminous Galaxies

AbstractWe detected significant Zeeman splitting in the 1667 MHz OH megamaser emission from four ultraluminous galaxies. These detections, in addition to being the first extragalactic detection of the Zeeman effect in an emission line, suggest that OH megamasers are excellent extragalactic magnetometers.

Dense molecular gas and starbursts in ultraluminous galaxies

1992 ◽  
Vol 387 ◽  
pp. L55 ◽  
Author(s):  
P. M. Solomon ◽  
D. Downes ◽  
S. J. E. Radford
Keyword(s):  
Molecular Gas ◽  
Ultraluminous Galaxies

Rotating Nuclear Rings and Extreme Starbursts in Ultraluminous Galaxies

1998 ◽  
Vol 507 (2) ◽  
pp. 615-654 ◽  
Author(s):  
D. Downes ◽  
P. M. Solomon
Keyword(s):  
Ultraluminous Galaxies

scholarly journals Warm ultraluminous galaxies in the IRAS survey - The transition from galaxy to quasar?

1988 ◽  
Vol 328 ◽  
pp. L35 ◽  
Author(s):  
D. B. Sanders ◽  
B. T. Soifer ◽  
J. H. Elias ◽  
G. Neugebauer ◽  
K. Matthews
Keyword(s):  
Ultraluminous Galaxies

scholarly journals Molecular gas in submillimetre-faint, star-forming ultraluminous galaxies at z > 1

2011 ◽  
Vol 415 (3) ◽  
pp. 2723-2743 ◽  
Author(s):  
C. M. Casey ◽  
S. C. Chapman ◽  
R. Neri ◽  
F. Bertoldi ◽  
I. Smail ◽  
...  
Keyword(s):  
Molecular Gas ◽  
Faint Star ◽  
Star Forming ◽  
Ultraluminous Galaxies

scholarly journals Low-Ionization Balqsos: Warm Ultraluminous Galaxies at High Redshifts

1999 ◽  
Vol 186 ◽  
pp. 475-478
Author(s):  
E. Egami
Keyword(s):  
Galaxy Mergers ◽  
Ultraluminous Galaxies

A decade ago Sanders et al. (1988a, b) proposed a possible QSO formation scenario as a sequence of Galaxy Mergers → Ultraluminous IR Galaxies (ULIRGs) → Warm ULIRGs → QSOs. Since then, this proposal has become a paradigm against which all the subsequent observations will be compared. Fortunately for us, this paradigm makes two specific predictions: that is, 1) ULIRGs are powered by hidden AGNs, and 2) ULIRGs should be more abundant at z ~ 2, where the comoving density of optically-selected QSOs is sharply peaking up.

scholarly journals Confirming a population of hot-dust dominated, star-forming, ultraluminous galaxies at high redshift

2009 ◽  
Vol 399 (1) ◽  
pp. 121-128 ◽  
Author(s):  
C. M. Casey ◽  
S. C. Chapman ◽  
R. J. Beswick ◽  
A. D. Biggs ◽  
A. W. Blain ◽  
...  
Keyword(s):  
High Redshift ◽  
Star Forming ◽  
Ultraluminous Galaxies
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