In a merging companion galaxy quasar radiation transforms the gas

Formation and gas dynamics of the inner regions of NGC 1365: clusters and gas-dominated centers of disk galaxies. I. The case of VV 114

Borodina, O., Williams, T. G., Sormani, M. C., Meidt, S. & Schinnerer, E. On the Tremaine–Weinberg method: how much can we trust gas tracers to measure pattern speeds? There was a meeting on Mon. Not. R. Astron. 524, 3437–3445 (2023) was published by the society.

Rong, Y. Gas-rich ultra-diffuse galaxies are originated from high specific angular momentum. Preprint at https://arxiv.org/abs/2404.00555 (2024).

Daddi, E. The evidence for cold-stream to hot-cream transition can be seen from groups and clusters. Astrophys. J. Lett. 955, L21)

Elmegreen, B. G., Galliano, E. & Alloin, D. Massive clusters in the inner regions of NGC 1365: cluster formation and gas dynamics in galactic bars. There are astrophys. J. 701,1297–1308.

Wang, E. et al. There were no differences between the central and satellite galaxies. I. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching. There are astrophys. J. 884, 51.

Bland-Hawthorn, J., Tepper-Garcia, T., Agertz, O. & Freeman, K. There is a rapid start to bars in the baryon-dominated centers of disk galaxies. There are astrophys. J. 947, 80 (2023).

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. Astrophys. J. 92, 94 is expected to happen over the years.

Zhid, M. J., fabricant, D. G., and Hwang were all part of the project. The scaling of stellar mass and central stellar velocity dispersion for quiescent galaxies at z < 0.7. There are astrophys. J. 832, 203 (2016).

J. A. and his co-authors collaborated on a book, entitled “Handbook of Material Handling.” ALMA reveals potential evidence for spiral arms, bars, and rings in high-redshift submillimeter galaxies. Astrophys. J. 876, 130 (2019).

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

Block, D. L. et al. Gravitational bar and spiral arm torques from Ks-band observations and implications for the pattern speeds. Astron. J. 128, 183–1199 was written in 2004.

Liang, Z.-Z., Wang, J., Gao, H., Ho, L. C. & Athanassoula, E. Connection between non-axisymmetric structures and neutral gas distribution in disk galaxies. Preprints can be found at arxiv.org/abs/2410.13595.

D, Liu, et al. published their report. PHANGS-JWST first results: stellar-feedback-driven excitation and dissociation of molecular gas in the starburst ring of NGC 1365? There are astrophys. J. Lett. 955, L 19 (2023)

The tail of the abundant dwarf galaxy population can be found in the ultradiffuse galaxies. Mon. Not. R. Astron. Soc. 459, L51–L55 (2016).

J. Falcn-Barroso is a writer. The project was called the SAURON project. Integral-field absorption and emission-line kinematics of 24 spiral galaxy bulges. The day was Mon. Not. R. Astron. Soc. 369, 529–566 (2006).

Cowie, L. L., Songaila, A., Hu, E. M. & Cohen, J. G. New insight on galaxy formation and evolution from Keck spectroscopy of the Hawaii deep fields. Astron. J. 112 was published in 1996.

Weinberger, R. et al. Simulating galaxy formation with black hole driven thermal and kinetic feedback. The day will be Monday. Not. R. Astron. Soc. 465, 3291–3308 (2017).

Bar and bulges in a radial shear flow come from Turbulent gas-rich disks. Astrophys. J. 968, 86 was written in 1994.

The star formation in the large millimetre/submillimetre array era is a high-redshift star. The Royal Society Open Science will be published in 2020.

Hayward, C. C. et al. The implications for the Fund are discussed in Submillimetre galaxies in aHierarchical Universe. Mon. Not. R. Astron. Soc. 428, 2529–2547 (2013).

Di Teodoro, E. M. & Fraternali, F. 3DBAROLO: a new 3D algorithm to derive rotation curves of galaxies. Mon. Not. R. astron Soc. 451, 3021–3033 (2015).

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? The day was Mon. Not. R. Astron. Soc. 518, 2511–2520 (2023).

P. van Dokkum is related to the author. The high stellar velocity dispersion is related to the ultra-diffuse galaxy Dragonfly 44. Astrophys. J. Lett., L6 was published in June.

Yang, X., Mo, H. J., van den Bosch, F. C. & Jing, Y. P. Calibration and use of a halo-based galaxy group finder. Mon. Not. R. Astron. The Soc. 356,1293–1307 was published in 2005.

Correa, C. A. et al. The stellar mass Tully–Fisher relation is consistent with SIDM. Mon. Not. R. Astron. 548, 3343–3343 (2025).

Volonteri, M., Haardt, F. & Madau, P. The assembly and merging history of supermassive black holes in hierarchical models of galaxy formation. Astrophys. J. 582, 559–573 (2003).

Yang, D., Yu, H.-B. & An, H. Self-interacting dark matter and the origin of ultradiffuse galaxies NGC1052-DF2 and -DF4. Phys. Rev. Lett. 125, 111105 (2020).

M. S., et al. published a monograph. Cosmological and idealized simulations of dark matter haloes with velocity-dependent, rare and frequent self-interactions. The day was Mon. Not. R. Astron. There is a report on the Soc. 518, 2327–1341 (2024).

Wang, H. et al. The local Universe has a reconstructed initial density field. III. The simulation in the volume was not good. Astrophys. J. 797, 163.

J., Wang, & Y.P. are related. halo assembly bias is related to the distribution of ejected subhaloes. There will be a meeting Mon. Not. R. Astron. The papers were issued in 396 and 2249.

A. D., Abramo, L. R., Prada, F., and Klypin, A. halo bias depends on age, concentration, and spin. Mon. Not. R. Astron. Soc. 487, 1570–1579 (2019).

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

Pillepich, A. et al. First results from the TNG50 simulation: the evolution of stellar and gaseous discs across cosmic time. Mon. Not. R. Astron. 490, 3196–3233 were published last year.

Kaplinghat, M., Tulin, S. & Yu, H.-B. Dark matter halos as particle colliders: unified solution to small-scale structure puzzles from dwarfs to clusters. 116, 040302, was published in the bulletin of the practictore lett.

Urrutia, T., Lacy, M. & Becker, R. H. Evidence for quasar activity triggered by galaxy mergers in HST observations of dust-reddened quasars. Astrophys. J. 674, 80–96 (2008).

A distant QSO-starburst system was caught by ALMA. There was a meeting on Mon. Not. R. Astron. Soc. 493, 3744–3756 (2020).

Y., Dubois, et al. The HORIZON-AGN simulation: morphological diversity of galaxies promoted by AGN feedback. Mon. Not. R. Astron. 386, 3948, and 3984 were written about in the Soc. 463.

The growth of black holes was the origin of antihierarchical growth. The day is Mon. Not. R. Astron. Soc. 426, 237–257 (2012).

Noterdaeme, P. et al. Take a sample of the quasar absorbers. Excess of damped H2 systems at zabs ≈ zQSO in SDSS DR14. Astron. Astrophys. 627, A32 (2019).

Rahmati, A. & Schaye, J. Predictions for the relation between strong Hi absorbers and galaxies at redshift 3. Mon. Not. R. Astron. Soc. 438, 529–547 (2014).

Noterdaeme, P. A connection between extremely strong damped Lyman-α systems and Lyman-α emitting galaxies at small impact parameters. Astron. Astrophys. 566, A24 (2014).

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. Astrophys. 457 was published in 2006

Balashev, S. A. et al. CO-dark molecular gas at high redshift: very large H2 content and high pressure in a low-metallicity damped Lyman alpha system. Mon. Not. R. Astron. Soc. 470, 2890–2910 (2017).

Directional radiation and photodissociation regions in the cloud of hydrogen. Astron. Lett. 35, 150–166 was published in 2009.

The number of emitting clouds in the broad-line region can be constrained by high-resolution spectroscopy of MRK 335. Mon. Not. R. Astron. There was an article in the sidebar about 1015–1020 in 1997.

Kosenko, D. N., Balashev, S. A. & Klimenko, V. V. Cold diffuse interstellar medium of Magellanic Clouds. II. The physical conditions at the time C I and H2 were experienced. Mon. Not. R. Astron. Soc. 528, 5065–5079 (2024).

C., Impey, C. D., Rix, H.-W. The images were analyzed and their decomposition was detailed. I. Beyond the aixysymmetric models. Astron. J. 139, 2097–2129 (2010).

Westmeier, T. et al. SOFIA 2 – an automated, parallel H i source finding pipeline for the WALLABY survey. Mon. Not. R. Astron. In the year 2021, Soc. 509, 3952–3962.

Evidence for multiple quenching mechanisms is attributed to the star formation histories of massive quiescent galaxies with Bagpipes. Mon. Not. R. Astron. 480, 4379–4401 was published in 2018).

Draine and Li had a glimpse of the red light from the dust. IV. The silicate-graphite- PAH model was used during the post-Spitzer era. There are astrophys. J. 663, 832, 832.

Sargent, M. T. et al. A description of the constant variation of gas properties in the mass-star formation plane is called regularity underlying complexity. There are astrophys. J. 793 was published in May of 2014).

Vestergaard, M. & Peterson, B. M. Determining central black hole masses in distant active galaxies and quasars. II. Improved optical and UV scaling relationships. Astrophys. J. 642, 694.

Selsing, J., Fynbo, J. P. U., Christensen, L. & Krogager, J. K. An X-shooter composite of bright 1 < z < 2 quasars from UV to infrared. Astron. Astrophys. 585, A87 (2016).

Wang, J., Hall, P. B., Ge, J., Li, A. & Schneider, D. P. Detections of the 2175 Å dust feature at 1.4 < z < 1.5 from the Sloan Digital Sky Survey. Astrophys. J. 609 was published in 2004.

Srianand, R., Gupta, N., Petitjean, P., Noterdaeme, P. & Saikia, D. J. Detection of the 2175 Å extinction feature and 21-cm absorption in two Mg ii systems at z ~ 1.3. It was Mon. Not. R. Astron. Soc. 391, L69–L73 (2008).

Gordon, K. D., Clayton, G. C., Misselt, K. A., Landolt, A. U. & Wolff, M. J. The Large Magellanic Cloud, and Small Magellanic Cloud were compared to the near- invisible extinction curves. Astrophys. J. 594, 279–293 (2003).

Kosenko, D. N. et al. HD Molecules have high red shift Cosmic Ray Ionizing Rate in the Interstellar Medium There was no meeting on Mon. Not. R. Astron. It’s the same as 3810–3822 for the year of 2021.

3Pj) fine structure states when hit with He. J. Phys. B: At. There was a person named Mol. The results of the 25th edition of the journal, Phys. 24, delivered in 1991.

Le Petit, F., Nehmé, C., Le Bourlot, J. & Roueff, E. A model for atomic and molecular interstellar gas: the Meudon PDR code. There are astrophys. There was a J. Suppl. Ser. 164, 506–529 (2006).

There is a Astropy Collaboration. They were 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. 955, 167.