scholarly journals A Tully-Fisher Relation for S0 Galaxies

1999 ◽  
Vol 117 (6) ◽  
pp. 2666-2675 ◽  
Author(s):  
Eyal Neistein ◽  
Dan Maoz ◽  
Hans-Walter Rix ◽  
John L. Tonry
Keyword(s):  
Fisher Relation ◽  
S0 Galaxies

The Tully-Fisher Relation in Coma and Virgo Cluster S0 Galaxies

2003 ◽  
Vol 126 (6) ◽  
pp. 2622-2634 ◽  
Author(s):  
J. L. Hinz ◽  
G. H. Rieke ◽  
N. Caldwell
Keyword(s):  
Virgo Cluster ◽  
Fisher Relation ◽  
S0 Galaxies

A Comparison of Coma Cluster S0 Galaxies with the Tully-Fisher Relation for Late-Type Spirals

2001 ◽  
Vol 121 (2) ◽  
pp. 683-691 ◽  
Author(s):  
Joannah L. Hinz ◽  
Hans-Walter Rix ◽  
Gary M. Bernstein
Keyword(s):  
Coma Cluster ◽  
Late Type ◽  
Fisher Relation ◽  
S0 Galaxies

scholarly journals The Tully–Fisher relation for S0 galaxies

2006 ◽  
Vol 373 (3) ◽  
pp. 1125-1140 ◽  
Author(s):  
A. G. Bedregal ◽  
A. Aragón-Salamanca ◽  
M. R. Merrifield
Keyword(s):  
Fisher Relation ◽  
S0 Galaxies

scholarly journals S0 galaxies in the Coma cluster: environmental dependence of the S0 offset from the Tully–Fisher relation

2013 ◽  
Vol 433 (3) ◽  
pp. 2667-2692 ◽  
Author(s):  
T. D. Rawle ◽  
John R. Lucey ◽  
Russell J. Smith ◽  
J. T. C. G. Head
Keyword(s):  
Coma Cluster ◽  
Fisher Relation ◽  
S0 Galaxies ◽  
Environmental Dependence

scholarly journals Formation of S0 galaxies through mergers

2014 ◽  
Vol 570 ◽  
pp. A103 ◽  
Author(s):  
Alejandro Borlaff ◽  
M. Carmen Eliche-Moral ◽  
Cristina Rodríguez-Pérez ◽  
Miguel Querejeta ◽  
Trinidad Tapia ◽  
...  
Keyword(s):  
S0 Galaxies

scholarly journals The multiwavelength Tully–Fisher relation with spatially resolved H i kinematics

2017 ◽  
Vol 469 (2) ◽  
pp. 2387-2400 ◽  
Author(s):  
Anastasia A. Ponomareva ◽  
Marc A. W. Verheijen ◽  
Reynier F. Peletier ◽  
Albert Bosma
Keyword(s):  
Spatially Resolved ◽  
Fisher Relation

scholarly journals A SLIPPERY SLOPE: SYSTEMATIC UNCERTAINTIES IN THE LINE WIDTH BARYONIC TULLY–FISHER RELATION

2016 ◽  
Vol 832 (1) ◽  
pp. 11 ◽  
Author(s):  
Jeremy D. Bradford ◽  
Marla C. Geha ◽  
Frank C. van den Bosch
Keyword(s):  
Line Width ◽  
Slippery Slope ◽  
Systematic Uncertainties ◽  
Fisher Relation

scholarly journals S0 galaxies are faded spirals: clues from their angular momentum content

2018 ◽  
Vol 476 (2) ◽  
pp. 2137-2167 ◽  
Author(s):  
Francesca Rizzo ◽  
Filippo Fraternali ◽  
Giuliano Iorio
Keyword(s):  
Angular Momentum ◽  
S0 Galaxies

scholarly journals Kinematics of the outskirts of S0 galaxies from PNe and GCs

2016 ◽  
Vol 11 (S321) ◽  
pp. 290-290
Author(s):  
A. Cortesi ◽  
C. Mendes de Oliveira
Keyword(s):  
Galaxy Formation ◽  
Globular Clusters ◽  
Velocity Dispersion ◽  
Spiral Galaxies ◽  
Formation Mechanisms ◽  
Stellar Kinematics ◽  
Lenticular Galaxies ◽  
Star Forming ◽  
Flat Rotation Curves ◽  
S0 Galaxies

AbstractThe stellar kinematics of the discs of S0 galaxies (as obtained using planetary nebulae, PNe, and integrated stellar light data) is comparable to that of spiral galaxies, with similar flat rotation curves and falling velocity dispersion profiles, but they present a larger amount of random motions. The only other tracer available to probe the kinematics of individual early-type galaxies are globular clusters (GCs). GCs’ formation is intimately connected to a galaxy major star forming event(s) and GCs are, therefore, good proofs of galaxy formation histories. We directly compare a sample of PNe, GCs, and stellar velocities out to 4 effective radii, in the S0 galaxies NGC 2768 and NGC 1023. In particular, we test a new method for studying GC properties and we find that these two lenticular galaxies are consistent with being formed through different formation mechanisms.

A new jet/outflow maser in the nucleus of the Compton-thick AGN IRAS 15480-0344

2017 ◽  
Vol 13 (S336) ◽  
pp. 129-132
Author(s):  
Paola Castangia ◽  
Andrea Tarchi ◽  
Alessandro Caccianiga ◽  
Paola Severgnini ◽  
Gabriele Surcis ◽  
...  
Keyword(s):  
Detection Rate ◽  
Radio Continuum ◽  
Continuum Emission ◽  
Maser Emission ◽  
X Ray ◽  
Vlbi Observations ◽  
S0 Galaxies ◽  
Water Maser

AbstractInvestigations of H2O maser galaxies at X-ray energies reveal that most harbor highly absorbed AGN. Possible correlations between the intrinsic X-ray luminosity and the properties of water maser emission have been suggested. With the aim of looking into these correlations on a more solid statistical basis, we have search for maser emission in a well-defined sample of Compton-thick AGN. Here we report the results of the survey, which yielded a surprisingly high maser detection rate, with a particular focus on the newly discovered luminous water maser in the lenticular (field) S0 galaxy IRAS 15480-0344. Recently, VLBI observations have been obtained to image the line and continuum emission in the nucleus of this galaxy. The radio continuum emission at VLBI scales is resolved into two compact components that are interpreted as jet knots. Based on the single-dish profile, the variability of the maser emission, and the position of the maser spots with respect to these continuum sources, we favor of a jet/outflow origin for the maser emission, consistent with similar cases found in other radio-quiet AGN. This scenario is consistent with the hypothesis of the presence of strong nuclear winds recently invoked to explain the main characteristics of field S0 galaxies.

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