Results 101 to 110 of about 6,612 (195)

The GALEX Ultraviolet Atlas of Nearby Galaxies [PDF]

, 2007
We present images, integrated photometry, and surface-brightness and color profiles for a total of 1034 nearby galaxies recently observed by the Galaxy Evolution Explorer (GALEX) satellite in its far-ultraviolet (FUV; λ_(eff) = 1516 Å) and near ...
Barlow, Tom A., Bianchi, Luciana, Boissier, Samuel, Boselli, Alessandro, Conrow, Tim, Donas, José, Forster, Karl, Friedman, Peter G., Gil de Paz, Armando, Heckman, Timothy M., Joe, Young H., Lee, Young-Wook, Madore, Barry F., Martin, D. Christopher, Milliard, Bruno, Morrissey, Patrick, Neff, Susan G., Rey, Soo-Chang, Rich, R. Michael, Schiminovich, David, Seibert, Mark, Small, Todd, Szalay, Alex S., Thilker, David, Wyder, Ted K., Yi, Sukyoung   +25 more
core  

Detection of a Star Forming Galaxy in the Center of a Low-Mass Galaxy Cluster

, 2018
Brightest Cluster Galaxies (BCGs) residing in the centers of galaxy clusters are typically quenched giant ellipticals. A recent study hinted that star-forming galaxies with large disks, so-called superluminous spirals and lenticulars, are the BCGs of a ...
Andrade-Santos, Felipe, Bogdan, Akos, Forman, William R., Jones, Christine, Kovacs, Orsolya E., Kraft, Ralph P., Lovisari, Lorenzo   +6 more
core   +1 more source

Exploring Lenticular Galaxy Formation in Field Environments Using NewHorizon: Evidence for Counterrotating Gas Accretion as a Formation Channel

The Astrophysical Journal
The formation pathways of lenticular galaxies (S0s) in field environments remain a matter of debate. We utilize the cosmological hydrodynamic simulation, NewHorizon , to investigate the issue. We select two massive star formation quenched S0s as our main
Seongbong Han, J. K. Jang, Emanuele Contini, Yohan Dubois, Seyoung Jeon, Sugata Kaviraj, Taysun Kimm, Katarina Kraljic, Sree Oh, Sébastien Peirani, Christophe Pichon, Sukyoung K. Yi   +11 more
doaj   +1 more source

Stars throw their weight in old galaxies

, 2012
The observation that old, massive galaxies have a larger fraction of low-mass stars than their younger, lower-mass counterparts adds to mounting evidence that star formation may have been different in the early Universe.Comment: Invited Nature "News and ...
Bastian, Nate
core   +1 more source

Knowledge-enhanced prototypical network with class cluster loss for few-shot relation classification. [PDF]

PLoS One, 2023
Liu T, Ke Z, Li Y, Silamu W.
europepmc   +1 more source

Toward Understanding the Evolutionary Role of Star-forming Lenticular Galaxies: New H i Detections and Comparison with Quiescent S0s and Red Spirals

The Astrophysical Journal
As one type of blue early-type galaxy, the evolutionary history and fate of star-forming lenticular galaxies (S0s) remain elusive. We selected 134 star-forming S0s from the Sloan Digital Sky Survey IV MaNGA survey and found that they have steep and ...
Pei-Bin Chen, Junfeng Wang, Tian-Wen Cao, Mengting Shen, Xiaoyu Xu   +4 more
doaj   +1 more source

The Cool ISM in S0 Galaxies. I. A Survey of Molecular Gas

, 2002
Lenticular galaxies remain remarkably mysterious as a class. Observations to date have not led to any broad consensus about their origins, properties and evolution, though they are often thought to have formed in one big burst of star formation early in ...
Appleton P. N., Arimoto N., Baugh C. M., Bekki K., Bekki K., Bieging J. H., Biermann P., Bottinelli L., Bower R. G., Buson L. M., Capaccioli M., Chamaraux P., Gary A. Welch, Gerin M., Huchtmeier W. K., Kauffmann G., Knapp G. R., Larson R. B., Leslie J. Sage, Madau P., Mihos J. C., Richter O.-G., Rocca-Volmerange B., Sage L. J., Sage L. J., Sage L. J., Sage L. J., Sancisi R., Shostak G. S., Tacconi L. J., van der Burg G., van Driel W., Veron-Cetty M.-P., White S. D. M., Wiklind T., Wiklind T., Wiklind T., Wiklind T.   +37 more
core   +2 more sources

The Invisibility of Scotomas I: The Carving Hypothesis. [PDF]

Optom Vis Sci, 2023
Peli E, Goldstein R, Jung JH.
europepmc   +1 more source

86th Annual Meeting of the Meteoritical Society (2024)

Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley   +1 more source

The Morphology - Density Relation in z ~ 1 Clusters

, 2005
We measure the morphology--density relation (MDR) and morphology-radius relation (MRR) for galaxies in seven z ~ 1 clusters that have been observed with the Advanced Camera for Surveys on board the Hubble Space Telescope.
A. R. Martel, B. Holden, C. Gronwall, C. J. Burrows, D. A. Golimowski, D. R. Ardila, Della Ceca R., E. S. Cheng, F. Bartko, F. Menanteau, G. D. Illingworth, G. F. Hartig, G. K. Miley, G. R. Meurer, Goto T., H. C. Ford, H. D. Tran, Icke V., J. E. Krist, J. P. Blakeslee, K.‐V. Tran, Kauffmann G., L. D. Bradley, L. Infante, M. Clampin, M. Franx, M. P. Lesser, M. Postman, M. Sirianni, N. Benitez, N. Homeier, N. J. G. Cross, P. D. Feldman, P. Rosati, Ponman T. J., R. A. Brown, R. A. Kimble, R. Demarco, R. J. Bouwens, R. L. White, S. Mei, T. Goto, T. J. Broadhurst, V. Motta, W. B. Sparks, W. Zheng, Z. I. Tsvetanov   +46 more
core   +1 more source