Zobrazeno 1 - 10
of 33
pro vyhledávání: '"S C O Glover"'
Autor:
Nina S Sartorio, A Fialkov, T Hartwig, G M Mirouh, R G Izzard, M Magg, R S Klessen, S C O Glover, L Chen, Y Tarumi, D D Hendriks
The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals, su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c0cc384ccd691420171211cdf5130e1d
Autor:
B Groves, K Kreckel, F Santoro, F Belfiore, E Zavodnik, E Congiu, O V Egorov, E Emsellem, K Grasha, A Leroy, F Scheuermann, E Schinnerer, E J Watkins, A T Barnes, F Bigiel, D A Dale, S C O Glover, I Pessa, P Sanchez-Blazquez, T G Williams
Ionized nebulae provide critical insights into the conditions of the interstellar medium (ISM). Their bright emission lines enable the measurement of physical properties, such as the gas-phase metallicity, across galaxy disks and in distant galaxies.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::15420537ac5cddebbd8edf58b157415d
Autor:
I. Pessa, E. Schinnerer, P. Sanchez-Blazquez, F. Belfiore, B. Groves, E. Emsellem, J. Neumann, A. K. Leroy, F. Bigiel, M. Chevance, D. A. Dale, S. C. O. Glover, K. Grasha, R. S. Klessen, K. Kreckel, J. M. D. Kruijssen, F. Pinna, M. Querejeta, E. Rosolowsky, T. G. Williams
Publikováno v:
Astronomy & Astrophysics. 673:A147
Analyzing resolved stellar populations across the disk of a galaxy can provide unique insights into how that galaxy assembled its stellar mass over its lifetime. Previous work at ~1 kpc resolution has already revealed common features in the mass buil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa90824875177252a7201b1ad01aeb08
https://doi.org/10.1051/0004-6361/202245673
https://doi.org/10.1051/0004-6361/202245673
Autor:
A. García-Rodríguez, A. Usero, A. K. Leroy, F. Bigiel, M. J. Jiménez-Donaire, D. Liu, M. Querejeta, T. Saito, E. Schinnerer, A. Barnes, F. Belfiore, I. Bešlić, Y. Cao, M. Chevance, D. A. Dale, J. S. den Brok, C. Eibensteiner, S. García-Burillo, S. C. O. Glover, R. S. Klessen, J. Pety, J. Puschnig, E. Rosolowsky, K. Sandstrom, M. C. Sormani, Y.-H. Teng, T. G. Williams
Publikováno v:
Astronomy & Astrophysics. 672:A96
We present new HCN and HCO$^+$ ($J$=3-2) images of the nearby star-forming galaxies (SFGs) NGC 3351, NGC 3627, and NGC 4321. The observations, obtained with the Morita ALMA Compact Array, have a spatial resolution of $\sim$290-440 pc and resolve the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::96a6412cedb07c9f848ea51d0379f984
https://doi.org/10.1051/0004-6361/202244317
https://doi.org/10.1051/0004-6361/202244317
Autor:
A. T. Barnes, R. Chandar, K. Kreckel, S. C. O. Glover, F. Scheuermann, F. Belfiore, F. Bigiel, G. A. Blanc, M. Boquien, J. den Brok, E. Congiu, M. Chevance, D. A. Dale, S. Deger, J. M. D. Kruijssen, O. V. Egorov, C. Eibensteiner, E. Emsellem, K. Grasha, B. Groves, R. S. Klessen, S. Hannon, H. Hassani, J. C. Lee, A. K. Leroy, L. A. Lopez, A. F. McLeod, H. Pan, P. Sánchez-Blázquez, E. Schinnerer, M. C. Sormani, D. A. Thilker, L. Ubeda, E. J. Watkins, T. G. Williams
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 662, ⟨10.1051/0004-6361/202243766⟩
A&A
Astronomy and Astrophysics-A&A, 2022, 662, ⟨10.1051/0004-6361/202243766⟩
A&A
One of the fundamental factors regulating the evolution of galaxies is stellar feedback. However, we still do not have strong observational constraints on the relative importance of the different feedback mechanisms (e.g. radiation, ionised gas press
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::61ed0f2e117ac15543722e53dcf0454b
Autor:
J. Wallace, C. Battersby, E. A. C. Mills, J. D. Henshaw, M. C. Sormani, A. Ginsburg, A. T. Barnes, H. P. Hatchfield, S. C. O. Glover, L. D. Anderson
Publikováno v:
The Astrophysical Journal. 939:58
We report on the discovery of linear filaments observed in CO(1-0) emission for a $\sim2'$ field of view toward the Sgr E star forming region centered at (l,b)=(358.720$^\circ$, 0.011$^\circ$). The Sgr E region is thought to be at the turbulent inter
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9b3bf71f33392ee455bed22cf564bc0
https://doi.org/10.3847/1538-4357/ac951a
https://doi.org/10.3847/1538-4357/ac951a
Autor:
Andreas Schruba, K. Kreckel, Takashi Saito, Patricia Sanchez-Blazquez, E. Emsellem, I-Ting Ho, F. Santoro, Frank Bigiel, M. Chevance, Brent Groves, Sharon E. Meidt, J. Pety, Karin Sandstrom, Erik Rosolowsky, G. Blanc, K. Grasha, Eva Schinnerer, Christopher M Faesi, Enrico Congiu, S. C. O. Glover, R. McElroy, Philipp Lang, J. M. D. Kruijssen, Adam K. Leroy
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2021, 912 (2), pp.167. ⟨10.3847/1538-4357/abf7c2⟩
The Astrophysical Journal, American Astronomical Society, 2021, 912 (2), pp.167. ⟨10.3847/1538-4357/abf7c2⟩
We have noticed an error in the radial metallicity gradient fits provided in Table 3 (Appendix C) of the published article. The columns that list the metallicity gradients have units of dex arcmin-1, rather than the noted dex kpc-1. In the following
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0f7596e095799922f8e50921e10e845
https://hal.archives-ouvertes.fr/hal-03501725
https://hal.archives-ouvertes.fr/hal-03501725
Autor:
Frank Bigiel, Brent Groves, Toshiki Saito, M. Querejeta, Annie Hughes, Christopher M Faesi, S. C. O. Glover, Ashley T. Barnes, Yixian Cao, M. Chevance, Daizhong Liu, Jonathan D. Henshaw, Eva Schinnerer, C. N. Herrera, Eric Emsellem, Guillermo A. Blanc, Andreas Schruba, J. M. Diederik Kruijssen, Thomas G. Williams, Elizabeth Watkins, K. Grasha, Jiayi Sun, R. S. Klessen, Erik Rosolowsky, Arjen Van der Wel, Hsi-An Pan, J. Pety, K. Kreckel, A. Usero, Daniel A. Dale, Adam K. Leroy, Sharon Meidt
Publikováno v:
ApJ
The Astrophysical Journal
The Astrophysical Journal, 2021, 913, 16 pp. ⟨10.3847/1538-4357/abf35b⟩
ASTROPHYSICAL JOURNAL
The Astrophysical Journal
The Astrophysical Journal, 2021, 913, 16 pp. ⟨10.3847/1538-4357/abf35b⟩
ASTROPHYSICAL JOURNAL
In this paper we examine the factors that shape the distribution of molecular gas surface densities on the 150 pc scale across 67 morphologically diverse star-forming galaxies in the PHANGS-ALMA CO (2-1) survey. Dividing each galaxy into radial bins,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e792723fb333d6cb6b47fcddd8de4fe
Autor:
Nirupam Roy, Steven N. Longmore, S. C. O. Glover, Juan D. Soler, Hendrik Linz, S. Rezaei Kh., J. Syed, S. Bialy, Jonathan D. Henshaw, Jeroen M. Stil, Juergen Ott, M. Riener, Paul F. Goldsmith, J. Kerp, Nicola Schneider, Y. M. Wang, Henrik Beuther, James Urquhart, S. Suri, Robert J. Smith, Ralf S. Klessen, Michael Rugel
Publikováno v:
A&A
Syed, J, Soler, J D, Beuther, H, Wang, Y, Suri, S, Henshaw, J D, Riener, M, Bialy, S, Rezaei Kh, S, Stil, J M, Goldsmith, P F, Rugel, M R, Glover, S C O, Klessen, R S, Kerp, J, Urquhart, J S, Ott, J, Roy, N, Schneider, N, Smith, R J, Longmore, S N & Linz, H 2022, ' The “Maggie” filament: Physical properties of a giant atomic cloud ', Astronomy & Astrophysics . https://doi.org/10.1051/0004-6361/202141265
Syed, J, Soler, J D, Beuther, H, Wang, Y, Suri, S, Henshaw, J D, Riener, M, Bialy, S, Rezaei Kh, S, Stil, J M, Goldsmith, P F, Rugel, M R, Glover, S C O, Klessen, R S, Kerp, J, Urquhart, J S, Ott, J, Roy, N, Schneider, N, Smith, R J, Longmore, S N & Linz, H 2022, ' The “Maggie” filament: Physical properties of a giant atomic cloud ', Astronomy & Astrophysics . https://doi.org/10.1051/0004-6361/202141265
The atomic phase of the interstellar medium plays a key role in the formation process of molecular clouds. Due to the line-of-sight confusion in the Galactic plane that is associated with its ubiquity, atomic hydrogen emission has been challenging to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39fa39e12953e564c9ab5800a235576b
Autor:
J. Pety, Eric J. Murphy, Andreas Schruba, Christopher M Faesi, S. C. O. Glover, Dyas Utomo, Sharon E. Meidt, Santiago García-Burillo, Eva Schinnerer, M. Chevance, Adam K. Leroy, Emmanuel Momjian, J. M. D. Kruijssen, Frank Bigiel, Alexander P. S. Hygate, M. Gallagher, A. Usero, Miguel Querejeta, M. J. Jimenez-Donaire, Erik Rosolowsky
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A19. ⟨10.1051/0004-6361/201834915⟩
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 625, pp.A19. ⟨10.1051/0004-6361/201834915⟩
Astronomy & Astrophysics
ASTRONOMY & ASTROPHYSICS
Astronomy and Astrophysics
It remains unclear what sets the efficiency with which molecular gas transforms into stars. Here we present a new VLA map of the spiral galaxy M51 in 33GHz radio continuum, an extinction-free tracer of star formation, at 3" scales (~100pc). We combin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7332237ddab7012f0d4e44c277a71683
https://hal.archives-ouvertes.fr/hal-03081719
https://hal.archives-ouvertes.fr/hal-03081719