Search Results - "Faesi, C."

New constraints on the 12CO(2–1)/(1–0) line ratio across nearby disc galaxies by den Brok, J S, Chatzigiannakis, D, Bigiel, F, Puschnig, J, Barnes, A T, Leroy, A K, Jiménez-Donaire, M J, Usero, A, Schinnerer, E, Rosolowsky, E, Faesi, C M, Grasha, K, Hughes, A, Kruijssen, J M D, Liu, D, Neumann, L, Pety, J, Querejeta, M, Saito, T, Schruba, A, Stuber, S

“…ABSTRACT Both the CO(2–1) and CO(1–0) lines are used to trace the mass of molecular gas in galaxies. Translating the molecular gas mass estimates between…”
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Mapping Metallicity Variations across Nearby Galaxy Disks by Kreckel, K., Ho, I.-T., Blanc, G. A., Groves, B., Santoro, F., Schinnerer, E., Bigiel, F., Chevance, M., Congiu, E., Emsellem, E., Faesi, C., Glover, S. C. O., Grasha, K., Kruijssen, J. M. D., Lang, P., Leroy, A. K., Meidt, S. E., McElroy, R., Pety, J., Rosolowsky, E., Saito, T., Sandstrom, K., Sanchez-Blazquez, P., Schruba, A.

“…The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution…”
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Dense molecular gas properties on 100 pc scales across the disc of NGC 3627 by Bešlić, I, Barnes, A T, Bigiel, F, Puschnig, J, Pety, J, Herrera Contreras, C, Leroy, A K, Usero, A, Schinnerer, E, Meidt, S E, Emsellem, E, Hughes, A, Faesi, C, Kreckel, K, Belfiore, F M C, Chevance, M, den Brok, J S, Eibensteiner, C, Glover, S C O, Grasha, K, Jimenez-Donaire, M J, Klessen, R S, Kruijssen, J M D, Liu, D, Pessa, I, Querejeta, M, Rosolowsky, E, Saito, T, Santoro, F, Schruba, A, Sormani, M C, Williams, T G

“…ABSTRACT It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required…”
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Erratum: “Mapping Metallicity Variations across Nearby Galaxy Disks” (2019, ApJ, 887, 80) by Kreckel, K., Ho, I.-T., Blanc, G. A., Groves, B., Santoro, F., Schinnerer, E., Bigiel, F., Chevance, M., Congiu, E., Emsellem, E., Faesi, C., Glover, S. C. O., Grasha, K., Kruijssen, J. M. D., Lang, P., Leroy, A. K., Meidt, S. E., McElroy, R., Pety, J., Rosolowsky, E., Saito, T., Sandstrom, K., Sanchez-Blazquez, P., Schruba, A.

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A sensitive, high-resolution, wide-field IRAM NOEMA CO(1-0) survey of the very nearby spiral galaxy IC 342 by Querejeta, M, Pety, J, Schruba, A, Leroy, A. K, Herrera, C. N, Chiang, I-D, Meidt, S. E, Rosolowsky, E, Schinnerer, E, Schuster, K, Sun, J, Herrmann, K. A, Barnes, A. T, Beslic, I, Bigiel, F, Cao, Y, Chevance, M, Eibensteiner, C, Emsellem, E, Faesi, C. M, Hughes, A, Kim, J, Klessen, R. S, Kreckel, K, Kruijssen, J. M. D, Liu, D, Neumayer, N, Pan, H. -A, Saito, T, Sandstrom, K, Teng, Y. -S, Usero, A, Williams, T. G, Zakardjian, A

“…A&A 680, A4 (2023) We present a new wide-field 10.75 x 10.75 arcmin^2 (~11x11 kpc^2), high-resolution (theta = 3.6" ~ 60 pc) NOEMA CO(1-0) survey of the very…”
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New Constraints on the $^{12}$CO(2-1)/(1-0) Line Ratio Across Nearby Disc Galaxies by Brok, J. S. den, Chatzigiannakis, D, Bigiel, F, Puschnig, J, Barnes, A. T, Leroy, A. K, Jiménez-Donaire, M. J, Usero, A, Schinnerer, E, Rosolowsky, E, Faesi, C. M, Grasha, K, Hughes, A, Kruijssen, J. M. D, Liu, D, Neumann, L, Pety, J, Querejeta, M, Saito, T, Schruba, A, Stuber, S

“…Both the CO(2-1) and CO(1-0) lines are used to trace the mass of molecular gas in galaxies. Translating the molecular gas mass estimates between studies using…”
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Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300 by Riener, M, Faesi, C. M, Forbrich, J, Lada, C. J

“…A&A 612, A81 (2018) We used multi-band observations by the Herschel Space Observatory to study the dust emission properties of the nearby spiral galaxy NGC…”
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Star formation scaling relations at ~100 pc from PHANGS: Impact of completeness and spatial scale by Pessa, I, Schinnerer, E, Belfiore, F, Emsellem, E, Leroy, A. K, Schruba, A, Kruijssen, J. M. D, Pan, H. -A, Blanc, G. A, Sanchez-Blazquez, P, Bigiel, F, Chevance, M, Congiu, E, Dale, D, Faesi, C. M, Glover, S. C. O, Grasha, K, Groves, B, Ho, I, Jiménez-Donaire, M, Klessen, R, Kreckel, K, Koch, E. W, Liu, D, Meidt, S, Pety, J, Querejeta, M, Rosolowsky, E, Saito, T, Santoro, F, Sun, J, Usero, A, Watkins, E. J, Williams, T. G

“…A&A 650, A134 (2021) Aims: The complexity of star formation at the physical scale of molecular clouds is not yet fully understood. We investigate the…”
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Dense gas is not enough: environmental variations in the star formation efficiency of dense molecular gas at 100pc scales in M51 by Querejeta, M, Schinnerer, E, Schruba, A, Murphy, E, Meidt, S, Usero, A, Leroy, A. K, Pety, J, Bigiel, F, Chevance, M, Faesi, C. M, Gallagher, M, García-Burillo, S, Glover, S. C. O, Hygate, A. P. S, Jiménez-Donaire, M. J, Kruijssen, J. M. D, Momjian, E, Rosolowsky, E, Utomo, D

“…A&A 625, A19 (2019) It remains unclear what sets the efficiency with which molecular gas transforms into stars. Here we present a new VLA map of the spiral…”
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Radial properties of dust in galaxies: Comparison between observations and isolated galaxy simulations by van der Giessen, S. A, Matsumoto, K, Relano, M, De Looze, I, Romano, L, Hirashita, H, Nagamine, K, Baes, M, Palla, M, Hou, K. C, Faesi, C

“…We study the importance of several processes that influence the evolution of dust and its grain size distribution on spatially resolved scales in nearby…”
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The Gas Morphology of Nearby Star-Forming Galaxies by Stuber, S. K, Schinnerer, E, Williams, T. G, Querejeta, M, Meidt, S, Emsellem, E, Barnes, A, Klessen, R. S, Leroy, A. K, Neumann, J, Sormani, M. C, Bigiel, F, Chevance, M, Dale, D, Faesi, C, Glover, S. C. O, Grasha, K, Kruijssen, J. M. D, Liu, D, Pan, H, Pety, J, Pinna, F, Saito, T, Usero, A, Watkins, E. J

“…A&A 676, A113 (2023) The morphology of a galaxy stems from secular and environmental processes during its evolutionary history. Thus galaxy morphologies have…”
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Stellar structures, molecular gas, and star formation across the PHANGS sample of nearby galaxies by Querejeta, M, Schinnerer, E, Meidt, S, Sun, J, Leroy, A. K, Emsellem, E, Klessen, R. S, Munoz-Mateos, J. C, Salo, H, Laurikainen, E, Beslic, I, Blanc, G. A, Chevance, M, Dale, D. A, Eibensteiner, C, Faesi, C, Garcia-Rodriguez, A, Glover, S. C. O, Grasha, K, Henshaw, J, Herrera, C, Hughes, A, Kreckel, K, Kruijssen, J. M. D, Liu, D, Murphy, E. J, Pan, H. -A, Pety, J, Razza, A, Rosolowsky, E, Saito, T, Schruba, A, Usero, A, Watkins, E. J, Williams, T. G

“…A&A 656, A133 (2021) We identify stellar structures in the PHANGS sample of 74 nearby galaxies and construct morphological masks of sub-galactic environments…”
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Dense molecular gas properties on 100 pc scales across the disc of NGC 3627 by Bešlić, I, Barnes, A. T, Bigiel, F, Puschnig, J, Pety, J, Contreras, C. Herrera, Leroy, A. K, Usero, A, Schinnerer, E, Meidt, S. E, Emsellem, E, Hughes, A, Faesi, C, Kreckel, K, Belfiore, F. M. C, Chevance, M, Brok, J. S. den, Eibensteiner, C, Glover, S. C. O, Grasha, K, Jimenez-Donaire, M. J, Klessen, R. S, Kruijssen, J. M. D, Liu, D, Pessa, I, Querejeta, M, Rosolowsky, E, Saito, T, Santoro, F, Schruba, A, Sormani, M. C, Williams, T. G

“…It is still poorly constrained how the densest phase of the interstellar medium varies across galactic environment. A large observing time is required to…”
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Mapping metallicity variations across nearby galaxy disks by Kreckel, K, Ho, I. -T, Blanc, G. A, Groves, B, Santoro, F, Schinnerer, E, Bigiel, F, Chevance, M, Congiu, E, Emsellem, E, Faesi, C, Glover, S. C. O, Grasha, K, Kruijssen, J. M. D, Lang, P, Leroy, A. K, Meidt, S. E, McElroy, R, Pety, J, Rosolowsky, E, Saito, T, Sandstrom, K, Sanchez-Blazquez, P, Schruba, A

“…The distribution of metals within a galaxy traces the baryon cycle and the buildup of galactic disks, but the detailed gas phase metallicity distribution…”
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A 50 pc scale view of star formation efficiency across NGC 628 by Kreckel, K, Faesi, C, Kruijssen, J. M. D, Schruba, A, Groves, B, Leroy, A. K, Bigiel, F, Blanc, G. A, Chevance, M, Herrera, C, Hughes, A, McElroy, R, Pety, J, Querejeta, M, Rosolowsky, E, Schinnerer, E, Sun, J, Usero, A, Utomo, D

“…Star formation is a multi-scale process that requires tracing cloud formation and stellar feedback within the local (<kpc) and global galaxy environment. We…”
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