Zobrazeno 1 - 10
of 788
pro vyhledávání: '"Boquien , Médéric"'
Autor:
Neumann, Lukas, Bigiel, Frank, Barnes, Ashley T., Gallagher, Molly J., Leroy, Adam, Usero, Antonio, Rosolowsky, Erik, Bešlić, Ivana, Boquien, Médéric, Cao, Yixian, Chevance, Mélanie, Colombo, Dario, Dale, Daniel A., Eibensteiner, Cosima, Grasha, Kathryn, Henshaw, Jonathan D., Jiménez-Donaire, María J., Meidt, Sharon, Menon, Shyam H., Murphy, Eric J., Pan, Hsi-An, Querejeta, Miguel, Saito, Toshiki, Schinnerer, Eva, Stuber, Sophia K., Teng, Yu-Hsuan, Williams, Thomas G.
The star formation rate (SFR) is tightly connected to the amount of dense gas in molecular clouds. However, it is not fully understood how the relationship between dense molecular gas and star formation varies within galaxies and in different morphol
Externí odkaz:
http://arxiv.org/abs/2406.12025
Autor:
Sutter, Jessica, Sandstrom, Karin, Chastenet, Jérémy, Leroy, Adam K., Koch, Eric W., Williams, Thomas G., Chown, Ryan, Belfiore, Francesco, Bigiel, Frank, Boquien, Médéric, Cao, Yixian, Chevance, Mélanie, Dale, Daniel A., Egorov, Oleg V., Glover, Simon C. O., Groves, Brent, Klessen, Ralf S., Kreckel, Kathryn, Larson, Kirsten L., Oakes, Elias K., Pathak, Debosmita, Ramambason, Lise, Rosolowsky, Erik, Watkins, Elizabeth J.
Polycyclic aromatic hydrocarbons (PAHs) are a ubiquitous component of the interstellar medium (ISM) in z~0 massive, star-forming galaxies and play key roles in ISM energy balance, chemistry, and shielding. Wide field of view, high resolution mid-infr
Externí odkaz:
http://arxiv.org/abs/2405.15102
Autor:
Floyd, Matthew, Chandar, Rupali, Whitmore, Bradley C., Thilker, David A., Lee, Janice C., Pauline, Rachel E., Thomas, Zion L., Berschback, William J., Henny, Kiana F., Dale, Daniel A., Klessen, Ralf S., Schinnerer, Eva, Grasha, Kathryn, Boquien, Mederic, Larson, Kirsten L., Deger, Sinan, Barnes, Ashley T., Leroy, Adam K., Rosolowsky, Erik, Williams, Thomas G., Ubeda, Leonardo
Publikováno v:
The Astronomical Journal, Volume 167, Issue 3, id.95, 16 pp. March 2024
We present new catalogs of likely globular clusters (GCs) in 17 nearby spiral galaxies studied as part of the PHANGS-HST Treasury Survey. The galaxies were imaged in five broad-band filters from the near-ultraviolet through the $I$ band. PHANGS-HST h
Externí odkaz:
http://arxiv.org/abs/2403.13908
Autor:
Maschmann, Daniel, Lee, Janice C., Thilker, David A., Whitmore, Bradley C., Deger, Sinan, Boquien, Mederic, Chandar, Rupali, Dale, Daniel A., Wofford, Aida, Hannon, Stephen, Larson, Kirsten L., Leroy, Adam K., Schinnerer, Eva, Rosolowsky, Erik W., Ubeda, Leonardo, Barnes, Ashley, Emsellem, Eric, Grasha, Kathryn, Groves, Brent, Kim, Hwihyun, Klessen, Ralf S., Kreckel, Kathryn, Levy, Rebecca C., Pinna, Francesca, Rodriguez, Jimena, Tian, Qiushi, Williams, Thomas G.
We present the largest catalog to-date of star clusters and compact associations in nearby galaxies. We have performed a V-band-selected census of clusters across the 38 spiral galaxies of the PHANGS-HST Treasury Survey, and measured integrated, aper
Externí odkaz:
http://arxiv.org/abs/2403.04901
Autor:
Killi, Meghana, Ginolfi, Michele, Popping, Gergö, Watson, Darach, Zamorani, Giovanni, Lemaux, Brian C., Fujimoto, Seiji, Faisst, Andreas, Bethermin, Matthieu, Romano, Michael, Fudamoto, Yoshinobu, Bardelli, Sandro, Boquien, Médéric, Carniani, Stefano, Dessauges-Zavadsky, Miroslava, Gruppioni, Carlotta, Hathi, Nimish, Ibar, Eduardo, Jones, Gareth C., Koekemoer, Anton M., Langan, Ivanna, Méndez-Hernández, Hugo, Sugahara, Yuma, Vallini, Livia, Vergani, Daniela
Galaxy morphology is shaped by stellar activity, feedback, gas and dust properties, and interactions with surroundings, and can therefore provide insight into these processes. In this paper, we study the spatial offsets between stellar and interstell
Externí odkaz:
http://arxiv.org/abs/2402.07982
Autor:
Baron, Dalya, Sandstrom, Karin M., Rosolowsky, Erik, Egorov, Oleg V., Klessen, Ralf S., Leroy, Adam K., Boquien, Médéric, Schinnerer, Eva, Belfiore, Francesco, Groves, Brent, Chastenet, Jérémy, Dale, Daniel A., Blanc, Guillermo A., Méndez-Delgado, José E., Koch, Eric W., Grasha, Kathryn, Chevance, Mélanie, Thilker, David A., Colombo, Dario, Williams, Thomas G., Pathak, Debosmita, Sutter, Jessica, Brown, Toby, Wu, John F., Peek, J. E. G., Emsellem, Eric, Larson, Kirsten L., Neumann, Justus
The PHANGS survey uses ALMA, HST, VLT, and JWST to obtain an unprecedented high-resolution view of nearby galaxies, covering millions of spatially independent regions. The high dimensionality of such a diverse multi-wavelength dataset makes it challe
Externí odkaz:
http://arxiv.org/abs/2402.04330
Autor:
Williams, Thomas G., Lee, Janice C., Larson, Kirsten L., Leroy, Adam K., Sandstrom, Karin, Schinnerer, Eva, Thilker, David A., Belfiore, Francesco, Egorov, Oleg V., Rosolowsky, Erik, Sutter, Jessica, DePasquale, Joseph, Pagan, Alyssa, Berger, Travis A., Anand, Gagandeep S., Barnes, Ashley T., Bigiel, Frank, Boquien, Médéric, Cao, Yixian, Chastenet, Jérémy, Chevance, Mélanie, Chown, Ryan, Dale, Daniel A., Deger, Sinan, Eibensteiner, Cosima, Emsellem, Eric, Faesi, Christopher M., Glover, Simon C. O., Grasha, Kathryn, Hannon, Stephen, Hassani, Hamid, Henshaw, Jonathan D., Jiménez-Donaire, María J., Kim, Jaeyeon, Klessen, Ralf S., Koch, Eric W., Li, Jing, Liu, Daizhong, Meidt, Sharon E., Méndez-Delgado, J. Eduardo, Murphy, Eric J., Neumann, Justus, Neumann, Lukas, Neumayer, Nadine, Oakes, Elias K., Pathak, Debosmita, Pety, Jérôme, Pinna, Francesca, Querejeta, Miguel, Ramambason, Lise, Romanelli, Andrea, Sormani, Mattia C., Stuber, Sophia K., Sun, Jiayi, Teng, Yu-Hsuan, Usero, Antonio, Watkins, Elizabeth J., Weinbeck, Tony D.
The exquisite angular resolution and sensitivity of JWST is opening a new window for our understanding of the Universe. In nearby galaxies, JWST observations are revolutionizing our understanding of the first phases of star formation and the dusty in
Externí odkaz:
http://arxiv.org/abs/2401.15142
Autor:
Hassani, Hamid, Rosolowsky, Erik, Koch, Eric W., Postma, Joseph, Nofech, Joseph, Corbould, Harrisen, Thilker, David, Leroy, Adam K., Schinnerer, Eva, Belfiore, Francesco, Bigiel, Frank, Boquien, Mederic, Chevance, Melanie, Dale, Daniel A., Egorov, Oleg V., Emsellem, Eric, Glover, Simon C. O., Grasha, Kathryn, Groves, Brent, Henny, Kiana, Kim, Jaeyeon, Klessen, Ralf S., Kreckel, Kathryn, Kruijssen, J. M. Diederik, Lee, Janice C., Lopez, Laura A., Neumann, Justus, Pan, Hsi-An, Sandstrom, Karin M., Sarbadhicary, Sumit K., Sun, Jiayi, Williams, Thomas G.
We present the Physics at High Angular resolution in Nearby GalaxieS (PHANGS)-AstroSat atlas, which contains ultraviolet imaging of 31 nearby star-forming galaxies captured by the Ultraviolet Imaging Telescope (UVIT) on the AstroSat satellite. The at
Externí odkaz:
http://arxiv.org/abs/2312.06031
Autor:
Teng, Yu-Hsuan, Chiang, I-Da, Sandstrom, Karin M., Sun, Jiayi, Leroy, Adam K., Bolatto, Alberto D., Usero, Antonio, Ostriker, Eve C., Querejeta, Miguel, Chastenet, Jeremy, Bigiel, Frank, Boquien, Mederic, Brok, Jakob den, Cao, Yixian, Chevance, Melanie, Chown, Ryan, Colombo, Dario, Eibensteiner, Cosima, Glover, Simon C. O., Grasha, Kathryn, Henshaw, Jonathan D., Jimenez-Donaire, Maria J., Liu, Daizhong, Murphy, Eric J., Pan, Hsi-An, Stuber, Sophia K., Williams, Thomas G.
Determining how galactic environment, especially the high gas densities and complex dynamics in bar-fed galaxy centers, alters the star formation efficiency (SFE) of molecular gas is critical to understanding galaxy evolution. However, these same phy
Externí odkaz:
http://arxiv.org/abs/2310.16037
Autor:
Agostino, Christopher J., Salim, Samir, Boquien, Médéric, Janowiecki, Steven, Salas, Héctor, Couto, Guillherme S.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023, stad3027
Despite powerful X-ray emission, some AGNs are known to either lack optical emission lines (so-called 'optically dull' AGNs) or have lines that fall on the star-forming branch of the BPT diagram ('misclassified' AGNs). Aperture effects have been prop
Externí odkaz:
http://arxiv.org/abs/2310.10719