Zobrazeno 1 - 10
of 227
pro vyhledávání: '"Böker, Torsten"'
Autor:
Lamperti, Isabella, Arribas, Santiago, Perna, Michele, Del Pino, Bruno Rodríguez, Circosta, Chiara, Pérez-González, Pablo G., Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, D'Eugenio, Francesco, Maiolino, Roberto, Übler, Hannah, Willott, Chris J., Bertola, Elena, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Kumari, Nimisha, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo
We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the brightest member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were o
Externí odkaz:
http://arxiv.org/abs/2406.10348
Autor:
Pérez-González, Pablo G., D`Eugenio, Francesco, del Pino, Bruno Rodríguez, Übler, Hannah, Maiolino, Roberto, Arribas, Santiago, Cresci, Giovanni, Lamperti, Isabella, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Willott, Christopher J., Böker, Torsten, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo, Barro, Guillermo, Costantin, Luca, Martín-Navarro, Ignacio, Dunlop, James S., Magee, Daniel
Feedback is the key physical mechanism regulating galaxy formation. Stars in galaxies form when baryons radiatively cool down and fall into gravitational wells. Eventually, star formation quenches as gas is depleted and/or perturbed by feedback proce
Externí odkaz:
http://arxiv.org/abs/2405.03744
Autor:
Fisher, Deanne B., Bolatto, Alberto D., Chisholm, John, Fielding, Drummond, Levy, Rebecca C., Tarantino, Elizabeth, Boyer, Martha L., Cronin, Serena A., Lopez, Laura A., Smith, J. D., Berg, Danielle A., Lopez, Sebastian, Veilleux, Sylvain, van der Werf, Paul P., Böker, Torsten, Boogaard, Leindert A., Lenkić, Laura, Glover, Simon C. O., Villanueva, Vicente, Mayya, Divakara, Lai, Thomas S. -Y., Dale, Daniel A., Emig, Kimberly L., Walter, Fabian, Relaño, Monica, De Looze, Ilse, Mills, Elisabeth A. C., Leroy, Adam K., Meier, David S., Herrera-Camus, Rodrigo, Klessen, Ralf S.
In this paper we study the filamentary substructure of 3.3 $\mu$m PAH emission from JWST/NIRCam observations in the base of the M82 star-burst driven wind. We identify plume-like substructure within the PAH emission with widths of $\sim$50 pc. Severa
Externí odkaz:
http://arxiv.org/abs/2405.03686
Autor:
Fahrion, Katja, Böker, Torsten, Perna, Michele, Beck, Tracy L., Maiolino, Roberto, Arribas, Santiago, Bunker, Andrew J., Charlot, Stephane, Ceci, Matteo, Cresci, Giovanni, De Marchi, Guido, Lützgendorf, Nora, Ulivi, Lorenzo
We present a detailed study of the centre of NGC4654, a Milky Way-like spiral galaxy in the Virgo cluster that has been reported to host a double stellar nucleus, thus promising a rare view of ongoing star cluster infall into a galaxy nucleus. Analys
Externí odkaz:
http://arxiv.org/abs/2404.08910
Autor:
Ji, Xihan, Übler, Hannah, Maiolino, Roberto, D'Eugenio, Francesco, Arribas, Santiago, Bunker, Andrew J., Charlot, Stéphane, Perna, Michele, Del Pino, Bruno Rodríguez, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Kumari, Nimisha, Lamperti, Isabella
We report the chemical abundance pattern of GS\_3073, a galaxy at $z=5.55$ which was previously confirmed to host an overmassive active black hole, by leveraging the detection of about 40 emission lines, combining JWST/NIRSpec observations and ground
Externí odkaz:
http://arxiv.org/abs/2404.04148
Autor:
Bohn, Thomas, Inami, Hanae, Togi, Aditya, Armus, Lee, Lai, Thomas S. -Y., Barcos-Munoz, Loreto, Song, Yiqing, Linden, Sean T., Surace, Jason, Bianchin, Marina, U, Vivian, Evans, Aaron S., Böker, Torsten, Malkan, Matthew A., Larson, Kirsten L., Stierwalt, Sabrina, Buiten, Victorine A., Charmandaris, Vassilis, Diaz-Santos, Tanio, Howell, Justin H., Privon, George C., Ricci, Claudio, van der Werf, Paul P., Aalto, Susanne, Hayward, Christopher C., Kader, Justin A., Mazzarella, Joseph M., Muller-Sanchez, Francisco, Sanders, David B.
We present James Webb Space Telescope (JWST) Integral Field Spectrograph observations of NGC 3256, a local infrared-luminous late-stage merging system with two nuclei about 1 kpc apart, both of which have evidence of cold molecular outflows. Using JW
Externí odkaz:
http://arxiv.org/abs/2403.14751
Autor:
Perna, Michele, Arribas, Santiago, Lamperti, Isabella, Pereira-Santaella, Miguel, Ulivi, Lorenzo, Böker, Torsten, Maiolino, Roberto, Bunker, Andrew J., Charlot, Stéphane, Cresci, Giovanni, Del Pino, Bruno Rodríguez, D'Eugenio, Francesco, Übler, Hannah, Fahrion, Katja, Ceci, Matteo
Arp 220 is the nearest ULIRG; it shows evidence of 100 pc-scale molecular outflows likely connected with galaxy-scale outflows traced by ionised and neutral gas. The two highly obscured nuclei of Arp 220 are the site of intense star formation, with e
Externí odkaz:
http://arxiv.org/abs/2403.13948
Autor:
Übler, Hannah, D'Eugenio, Francesco, Perna, Michele, Arribas, Santiago, Jones, Gareth C., Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, Maiolino, Roberto, del Pino, Bruno Rodríguez, Willott, Chris J., Böker, Torsten, Cresci, Giovanni, Kumari, Nimisha, Lamperti, Isabella, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo
We present rest-frame optical data of the z~4 sub-millimeter galaxy GN20 obtained with JWST/NIRSpec in integral field spectroscopy (IFS) mode. The H$\alpha$ emission is asymmetric and clumpy and extends over a projected distance of more than 15 kpc.
Externí odkaz:
http://arxiv.org/abs/2403.03192
Autor:
Bolatto, Alberto D., Levy, Rebecca C., Tarantino, Elizabeth, Boyer, Martha L., Fisher, Deanne B., Leroy, Adam K., Cronin, Serena A., Klessen, Ralf S., Smith, J. D., Berg, Dannielle A., Boeker, Torsten, Boogaard, Leindert A., Ostriker, Eve C., Thompson, Todd A., Ott, Juergen, Lenkic, Laura, Lopez, Laura A., Dale, Daniel A., Veilleux, Sylvain, van der Werf, Paul P., Glover, Simon C. O., Sandstrom, Karin M., Skillman, Evan D., Chisholm, John, Villanueva, Vicente, Lai, Thomas S. -Y., Lopez, Sebastian, Mills, Elisabeth A. C., Emig, Kimberly L., Armus, Lee, Maya, Divakara, Meier, David S., De Looze, Ilse, Herrera-Camus, Rodrigo, Walter, Fabian, Relano, Monica, Koziol, Hannah B., Marvil, Joshua, Jimenez-Donaire, Maria J., Martini, Paul
We present new observations of the central 1 kpc of the M 82 starburst obtained with the James Webb Space Telescope (JWST) near-infrared camera (NIRCam) instrument at a resolution ~0.05"-0.1" (~1-2 pc). The data comprises images in three mostly conti
Externí odkaz:
http://arxiv.org/abs/2401.16648
Autor:
Übler, Hannah, Maiolino, Roberto, Pérez-González, Pablo G., D'Eugenio, Francesco, Perna, Michele, Curti, Mirko, Arribas, Santiago, Bunker, Andrew, Carniani, Stefano, Charlot, Stéphane, Del Pino, Bruno Rodríguez, Baker, William, Böker, Torsten, Cresci, Giovanni, Dunlop, James, Grogin, Norman A., Jones, Gareth C., Kumari, Nimisha, Lamperti, Isabella, Laporte, Nicolas, Marshall, Madeline A., Mazzolari, Giovanni, Parlanti, Eleonora, Rawle, Tim, Scholtz, Jan, Venturi, Giacomo, Witstok, Joris
A surprising finding of recent studies is the large number of Active Galactic Nuclei (AGN) associated with moderately massive black holes ($\rm \log(M_\bullet/M_\odot)\sim 6-8$), in the first billion years after the Big Bang ($z>5$). In this context,
Externí odkaz:
http://arxiv.org/abs/2312.03589