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The gas flow was driven by a bar in the Universe

Towards the theory of stellar-mass patterns in IR-dominated disk galaxies: clusters in the inner regions of NGC 1365

Williams, G. et al. The study of stellar-mass-based pattern speeds and comparisons with ISM kinematics has been applied to nearby galaxies. Astron. J. 161, 185 will take place over the course of a decade.

Villa-Vargas, J., Shlosman, I. & Heller, C. Dark matter halos and evolution of bars in disk galaxies: varying gas fraction and gas spatial resolution. There are astrophys. J. 719, 1470–1480 (2010).

Daddi, E. Evidence for cold-stream to hot-accretion transition as traced by Lyα emission from groups and clusters at 2 < z < 3.3. Astrophys. J. Lett. 928, L21 was released in 22nd century.

Elmegreen, B. G., Galliano, E. & Alloin, D. Massive clusters in the inner regions of NGC 1365: cluster formation and gas dynamics in galactic bars. Astrophys. J. 703 was published in 2009.

Wechsler, R. H., Zentner, A. R., Bullock, J. S., Kravtsov, A. V. & Allgood, B. The dependence of halo clustering on halo formation history, concentration, and occupation. Astrophys. J. 652, 71–84 (2006).

Díaz-García, S., Salo, H., Laurikainen, E. & Herrera-Endoqui, M. Characterization of galactic bars from 3.6 μm S4G imaging. Astron. 587 is an astrophys.

Mizukoshi, S. et al. Physical characterization of serendipitously uncovered millimeter-wave line-emitting galaxies at z 2.5 behind the local luminous infrared galaxy VV 114. There are astrophys. J. 917, 94 (2021).

J., Zahid, M. J., Fabricant, D G. The scaling of stellar mass and central stellar velocity dispersion for quiescent galaxies at z < 0.7. Astrophys. J. 832, 203 (2016).

Erwin, P. The frequency and sizes of inner bars and nuclear rings in barred galaxies and their dependence on galaxy properties. Mon. Not. R. Astron. 327, Soc. 528, 3613–3616 (2024).

A numerical study of interactions and stellar bars. Mon. Not. R. Astron. Soc. 464, 1502–1511 (2017).

Block, D. L. Gravitational bar and spiral arm torques from Ks-band observations and implications for the pattern speeds. Astron. J. 128, 183–201 (2004).

The relation between non-Axisymmetric structures and neutral gas distribution in the disk galaxies was studied. There is a preprint on this website at http://arxiv.org/abs/2410.13595

D. et al. PHANGS-JWST first results: stellar-feedback-driven excitation and dissociation of molecular gas in the starburst ring of NGC 1365? Astrophys. J. Lett. 944 and L19 are available.

Kormendy, J. & Kennicutt Jr, R. C. Secular evolution and the formation of pseudobulges in disk galaxies. There is a person named Annu. Rev. Astron. Astrophys. 42, 603–683 (2004).

Falcón-Barroso, J. et al. The project is called the Saulon. Integral-field absorption and emission-line kinematics of 24 spiral galaxy bulges. Mon. Not. R. Astron. 353, 355, 395, 411, 411, 411, 411, 411, 411.

New insight on galaxy formation and evolution from a deep field survey in Hawaii. Astron. J. 112 was published in 1996.

Goulding, A. D. Galaxy interactions trigger rapid black hole growth: an unprecedented view from the Hyper Suprime-Cam survey. Publ. Astron. Soc. Jpn 70, S37 (2018).

Turbulent gas-rich disks at high redshift have bars and bulges. Astrophys. J. 962, 86 (2024).

Hodge, J. A. & da Cunha, E. High-redshift star formation in the Atacama large millimetre/submillimetre array era. The Royal Society launched Open Science in 2005.

Hayward, C. C. et al. Submillimetre galaxies in a hierarchical universe: number counts, redshift distribution and implications for the IMF. The day was Mon. Not. R. Astron. 431, 2529, and 2547 were published this year.

Di Teodoro, E. M. & Fraternali, F. 3DBAROLO: a new 3D algorithm to derive rotation curves of galaxies. Mon. Not. R. Astron. The report was published on the society’s website, on June 8, 2015, at 3022–1033.

Lovell, C. C., Harrison, I., Harikane, Y., Tacchella, S. & Wilkins, S. M. Extreme value statistics of the halo and stellar mass distributions at high redshift: are JWST results in tension with ΛCDM? It’s Mon. Not. R. Astron. Soc. 518, 2511–2520 (2023).

van Dokkum, P. et al. A high stellar velocity dispersion and ~100 globular clusters for the ultra-diffuse galaxy Dragonfly 44. There are astrophys. J. Lett. 828, L6 (2016).

H. J., X., Mo, & F. C. were all present at the event. A halo-based galaxy group finder: calibration and application to the 2dFGRS. It was Mon. Not. R. Astron. Soc. 356, 1293–1307 (2005).

Mo, H. J. & Mao, S. The Tully–Fisher relation and its implications for the halo density profile and self-interacting dark matter. Mon. Not. There is R. Astron. There is a report about this issue in the Soc. 318, 163–172.

Ayromlio, M. Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations. There was no activity on Mon. Not. There is an R. Astron. The results of the Soc. 499, 1051–1069, and 1052–1069 in the coming years.

Dark matter and the origin of ultradiffuse galaxies. Phys. Rev. Lett. 125, 111105 (2020).

M. S., et al. are related. Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions. A day on Mon. Not. R. Astron. In case you’re wondering, it’s the university’s code of ethics, Soc. 529.

Wang, H., Mo, H. J., Yang, X., Jing, Y. P. & Lin, W. P. ELUCID—exploring the local Universe with the reconstructed initial density field. I. Hamiltonian Markov chain Monte Carlo method with particle mesh dynamics. Astrophys. J. 794, 94 (2014).

Wang, H., Mo, H. J. & Jing, Y. P. The distribution of ejected subhaloes and its implication for halo assembly bias. Mon. Not. R. Astron. Soc. 396, 2249–2256 (2009).

Sato-Polito, G., Montero-Dorta, A. D., Abramo, L. R., Prada, F. & Klypin, A. halo bias is related to age, concentration, and spin. The day will start on Mon. Not. R. Astron. Soc. 487, 1570–1579 (2019).

Marinacci, F. et al. First results from the IllustrisTNG simulations: radio haloes and magnetic fields. Mon. Not. R. Astron. Soc. 480, 5113–5139 (2018).

There are a number of articles contained in Pillepich et al. The first results of the simulation show how stellar and gaseous discs evolved over time. The day starts at 9:00 am Mon. Not. R. Astron. 490, 3196, and 3233 were published in 2019.

Kaplinghat, M., Tulin, S. & Yu, H.-B. Dark matter halos as particle colliders: unified solution to small-scale structure puzzles from dwarfs to clusters. Phys. Rev. Lett. 116, 041302 (2016).

Hopkins, P. F., Hernquist, L., Cox, T. J. & Kereš, D. A cosmological framework for the co-evolution of quasars, supermassive black holes, and elliptical galaxies. The activity of the quasar. Astrophys. It was J. Suppl. Ser. 175, 355–389 were posted in 2008.

Fogasy, J., Knudsen, K. K., Drouart, G., Lagos, C. D. P. & Fan, L. SMM J04135+10277: a distant QSO-starburst system caught by ALMA. There was a discussion about Mon. Not. R. Astron. In 2020 you can find Soc. 493 and 3744.

Dubois, Y. et al. The AGN feedback encourages morphological diversity of the galaxies. Mon. Not. R. Astron. Soc. 463, 3948–3964 (2016).

Hirschmann, M., Somerville, R. S., Naab, T. & Burkert, A. Origin of the antihierarchical growth of black holes. Mon. Not. R. Astron. This was written in the year 2012

Noterdaeme, P. et al. Discovery of a Perseus-like cloud in the early Universe. Carbon monoxide and small dust grains at zabs are towards the quasar J0000+0048. Astron. The title of the book is Astrophys.

Krogager, J.-K. et al. The NH i – Z distribution was reproduced by a model that was damped. It will be on Mon. Not. R. Astron. 499, 3014 and 2020

Krogager, J. K., Møller, P., Fynbo, J. P. U. & Noterdaeme, P. Consensus report on 25 yr of searches for damped Ly α galaxies in emission: confirming their metallicity-luminosity relation at z ≳ 2. There was no work on Mon. Not. R. Astron. Soc. 469, 2959–2981 (2017).

Ledoux, C., Petitjean, P., Fynbo, J. P. U., Møller, P. & Srianand, R. Velocity-metallicity correlation for high-z DLA galaxies: evidence of a mass-metallicity relation? Astron. There are astrophys.

Boissé, P. et al. A far UV study of interstellar gas towards HD 34078: high excitation H2 and small scale structure. Astron. 429, 509, and 525 were published in 2005.

Sternberg, A., Le Petit, F., Roueff, E. & Le Bourlot, J. H i-to-H2 transitions and H i column densities in galaxy star-forming regions. Astrophys. J. 790, 10 (2014).

In Arav, N. Barlow, T A. Laor and R. D. Blandford, constraints on the number of clouds in the broad-line region were studied with high-resolution spectroscopy of MRK 335. Mon. Not. R. Astron. There was a case in the society of Soc. 288, 1015–1206.

Kosenko, D. N., Balashev, S. A. & Klimenko, V. V. Cold diffuse interstellar medium of Magellanic Clouds. II. Physical conditions from excitation of C i and H2. The day was Mon. Not. R. Astron. Soc. 528, 5065–5079 (2024).

P., Ho, L.C., Impey, C. D., Rix, h.-W. Detailed analysis of the images from the universe. II. Beyond a few models. Astron. J. 140, 190, 209-229.

Westmeier, T. and a few others. SOFIA 2 – an automated, parallel H i source finding pipeline for the WALLABY survey. There was a Monday. Not. R. Astron. Soc. 506, 3962–3976 (2021).

Inferring the star formation histories of massive quiescent galaxies with Bagpipes: evidence for multiple quenching mechanisms. It was Mon. Not. There is R. Astron. Soc. 480, 4379–4401 (2018).

Draine and Li analysed the emission of the white light from the dust. IV. The silicate-graphite-PAH model in the post-Spitzer era. Astrophys. J. 657, 810–837 (2007).

Sargent, M. T. et al. Regularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate plane. Astrophys. J. 793, 19 (2014).

Vestergaard, M. & Peterson, B. M. Determining central black hole masses in distant active galaxies and quasars. II. Improved optical and UV scaling relationships. There are astrophys. J. 641 was published in 2006

An X-shooting sample of bright 1 Z 2 quasars from UV to IR were measured. Astron. Astrophys. 585, A87 (2016).

There were detections of the 2175 dust feature at a rate of 1.5 per second. There are astrophys. J. 609, 589–596 (2004).

Noterdaeme, P. et al. Spotting high-z molecular absorbers using neutral carbon. There was a complete survey with the VLT. Astron. The title of the article is Astrophys.

Gordon, K. D., Clayton, G. C., Misselt, K. A., Landolt, A. U. & Wolff, M. J. A quantitative comparison of the Small Magellanic Cloud, Large Magellanic Cloud, and Milky Way ultraviolet to near-infrared extinction curves. Astrophys. J. 594 was published in 2003

D. N. Kosenko, et al. HD molecules at high redshift: cosmic ray ionization rate in the diffuse interstellar medium. There was a meeting on Mon. Not. R. Astron. This year, 395, 3810, and 3810, will be taken into account.

A fine-structure effect of O i and C i on atomic hydrogen. There are astrophys. J. 654, 1171–1174 (2007).

Le Petit, Nehmé, C., and Le Bourlot are authors of the Meudon PDR code. There are astrophys. J. Suppl. Ser. 164, 506–529 (2006).

There is a collaboration between astronomy and astrology. et al. The Astropy Project: sustaining and growing a community-oriented open-source project and the latest major release (v5.0) of the core package. Astrophys. J. 935, 167 (2022).