Results 231 to 240 of about 744 (267)

Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe

Pérez-González P, D'Eugenio F, Pino BRD, Perna M, Uebler H, Maiolino R, Arribas S, Lamperti I, Bunker A, Carniani S, Charlot S, Willott C, Böker T, Parlanti E, Scholtz J, Venturi G, Barro G, Costantin L, Navarro IM, Dunlop J, Magee D, Cresci G.   +21 more
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Lense-Thirring precession after a supermassive black hole disrupts a star. [PDF]

Nature
Pasham DR, Zajaček M, Nixon CJ, Coughlin ER, Śniegowska M, Janiuk A, Czerny B, Wevers T, Guolo M, Ajay Y, Loewenstein M.   +10 more
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Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback

Eckert D, Gastaldello F, Lovisari L, McGee S, Pasini T, Brienza M, Kolokythas K, O'Sullivan E, Simionescu A, Sun M, Bourne M, Chen Y, Cui W, Ettori S, Finoguenov A, Gozaliasl G, Kale R, Mernier F, Oppenheimer B, Schellenberger G, Seppi R, Tempel E.   +21 more
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Stellar content and kinematics of starburst galaxies

AIP Conference Proceedings, 1997
We present the Far Ultraviolet (FUV) spectra of four nearby starburst galaxies. We analyse them in terms of the stellar content and the kinematics of the interstellar medium and we discuss the implications of these results for the interpretation of the UV spectra of high redshift galaxies.
Rosa M. González Delgado, Claus Leitherer, Timothy Heckman   +2 more
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Higas and stellar content of early-type galaxies

New Astronomy Reviews, 2007
We present Australian telescope compact array observations of the neutral-hydrogen gas in 42 early-type galaxies detected by the HIPASS survey. We confirm the detection of 18 galaxies with Hi mass between a few times 10(9) and similar to 10(10)M(circle dot) and column density below a few times 10(20) cm(-2).
Serra, P., Trager, S. C., van der Hulst, J. M., Oosterloo, T. A., Morganti, R., van Gorkom, J. H., Sadler, E. M.   +6 more
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The stellar content of a prototype double barred galaxy

Astrophysics and Space Science, 2003
High spatial resolution visible and NIR observations of the bar of NGC 5850, a prototype of double barred spirals, together with visible intermediate and high dispersion spectra along the primary bar, are being used, with the aid of simple stellar population synthesis models, to investigate the mean age and metallicity of the different stellar ...
S. Lourenso, J. A. L. Aguerri, A. Vazdekis, J. E. Beckman, R. F. Peletier   +4 more
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Stellar content of the metal-poor galaxy DDO 68

Astronomy Letters, 2014
Based on archival Hubble Space Telescope ACS/WFC images, we have performed stellar photometry for the metal-poor galaxy DDO 68. The apparent distributions of stars of different ages and stellarmetallicity determinations indicate that DDO68 is a systemof two galaxies that have different stellar metallicities (Z = 0.004 and 0.001) and are in the stage of
N. A. Tikhonov, O. A. Galazutdinova, V. S. Lebedev   +2 more
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Elliptical galaxies : structure, stellar content, and evolution

1998
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in .pdf document. A near-infrared imaging survey of 341 nearby early-type galaxies, combined with optical imaging and spectroscopic data from the literature, are used to construct the global scaling relations for this population of galaxies.
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The stellar content of nuclear star clusters in spiral galaxies

SPIE Proceedings, 2003
We discuss first results from a spectroscopic survey of nuclear star clusters in nearby, late-type spiral galaxies. The data, obtained with the Space Telescope Imaging Spectrograph (STIS), allow us to derive cluster ages via stellar population synthesis methods.
Torsten Boeker, Roeland P. van der Marel, Joris Gerssen, Jakob Walcher, Hans-Walter Rix, Joseph C. Shields, Luis C. Ho   +6 more
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The stellar content of the A496 cD galaxy

Astronomy & Astrophysics, 1985
J, H, and K radial color distributions obtained for the galaxy A496 cD indicate that while the halo becomes bluer at increasing radii in the B-V, it becomes redder in the visual-IR colors. The combined visual-IR data lead to a unique model for both the main sequence and giant stars in which the main sequence is characterized by a radial increase of an ...
Valentijn, E. A., Moorwood, A. F. M.
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