Zobrazeno 1 - 10
of 35
pro vyhledávání: '"Lenkic, Laura"'
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:
Habel, Nolan, Nally, Conor, Lenkic, Laura, Meixner, Margaret, De Marchi, Guido, Kavanagh, Patrick J., Fahrion, Katja, Nayak, Omnarayani, Hirschauer, Alec S., Jones, Olivia C., Biazzo, Katia, Brandl, Bernhard R., Jaspers, Jeroen, Pontoppidan, Klaus M., Robberto, Massimo, Rogers, Ciaran, Sabbi, Elena, Sargent, B. A., Soderblom, David R., Zeidler, Peter
We present a JWST imaging survey with NIRCam and MIRI of NGC 346, the brightest star-forming region in the Small Magellanic Cloud (SMC). By combining aperture and point spread function (PSF) photometry of eleven wavelength bands across these two inst
Externí odkaz:
http://arxiv.org/abs/2404.16242
Autor:
Hirschauer, Alec S., Crouzet, Nicolas, Habel, Nolan, Lenkić, Laura, Nally, Conor, Jones, Olivia C., Bortolini, Giacomo, Boyer, Martha L., Meixner, Kay Justtanont Margaret, Östlin, Göran, Wright, Gillian S., Azzollini, Ruyman, Blommaert, Joris A. D. L., Brandl, Bernhard, Decin, Leen, Nayak, Omnarayani, Royer, Pierre, Sargent, B. A., van der Werf, Paul
We present a JWST imaging survey of I Zw 18, the archetypal extremely metal-poor, star-forming (SF), blue compact dwarf galaxy. With an oxygen abundance of only $\sim$3% $Z_{\odot}$, it is among the lowest-metallicity systems known in the local Unive
Externí odkaz:
http://arxiv.org/abs/2403.06980
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:
Nally, Conor, Jones, Olivia C., Lenkić, Laura, Habel, Nolan, Hirschauer, Alec S., Meixner, Margaret, Kavanagh, P. J., Boyer, Martha L., Ferguson, Annette M. N., Sargent, B. A., Nayak, Omnarayani, Temim, Tea
NGC 6822 is a nearby (~490 kpc) non-interacting low-metallicity (0.2 Zsolar) dwarf galaxy which hosts several prominent H ii regions, including sites of highly embedded active star formation. In this work, we present an imaging survey of NGC 6822 con
Externí odkaz:
http://arxiv.org/abs/2309.13521
Autor:
Lenkić, Laura, Nally, Conor, Jones, Olivia C., Boyer, Martha L., Kavanagh, Patrick J., Habel, Nolan, Nayak, Omnayarani, Hirschauer, Alec S., Meixner, Margaret, Sargent, B. A., Temim, Tea
We present an imaging survey of the Spitzer I star-forming region in NGC 6822 conducted with the NIRCam and MIRI instruments onboard JWST. Located at a distance of 490 kpc, NGC 6822 is the nearest non-interacting low-metallicity ($\sim$0.2 $Z_{\odot}
Externí odkaz:
http://arxiv.org/abs/2307.15704
Autor:
Lenkić, Laura, Bolatto, Alberto D., Fisher, Deanne B., Abraham, Roberto, Glazebrook, Karl, Herrera-Camus, Rodrigo, Levy, Rebecca C., Obreschkow, Danail, Volpert, Carolyn G.
The spectral line energy distribution of carbon monoxide contains information about the physical conditions of the star forming molecular hydrogen gas; however, the relation to local radiation field properties is poorly constrained. Using ~ 1-2 kpc s
Externí odkaz:
http://arxiv.org/abs/2301.05251
Autor:
Jones, Olivia C., Nally, Conor, Habel, Nolan, Lenkić, Laura, Fahrion, Katja, Hirschauer, Alec S., Chu, Laurie E. U., Meixner, Margaret, De Marchi, Guido, Nayak, Omnarayani, Robberto, Massimo, Sabbi, Elena, Zeidler, Peter, de Oliveira, Catarina Alves, Beck, Tracy, Biazzo, Katia, Brandl, Bernhard, Giardino, Giovanna, Jerabkova, Teresa, Keyes, Charles, Muzerolle, James, Panagia, Nino, Pontoppidan, Klaus M., Rogers, Ciaran, Sargent, B. A., Soderblom, David R.
JWST observations of NGC 346, a star-forming region in the metal-poor Small Magellanic Cloud, reveal a substantial population of sub-solar mass young stellar objects (YSOs) with IR excess. We detected $\sim$500 YSOs and pre main sequence (PMS) stars
Externí odkaz:
http://arxiv.org/abs/2301.03932
Autor:
Chu, Bronwyn Reichardt, Fisher, Deanne B., Bolatto, Alberto D., Chisholm, John, Fielding, Drummond, Berg, Danielle, Cameron, Alex J., Glazebrook, Karl, Herrera-Camus, Rodrigo, Kacprzak, Glenn G., Lenkić, Laura, Li, Miao, McPherson, Daniel K., Nielsen, Nikole M., Obreschkow, Danail, Vaught, Ryan J. Rickards, Sandstrom, Karin
We compare 500~pc scale, resolved observations of ionised and molecular gas for the $z\sim0.02$ starbursting disk galaxy IRAS08339+6517, using measurements from KCWI and NOEMA. We explore the relationship of the star formation driven ionised gas outf
Externí odkaz:
http://arxiv.org/abs/2211.02063
Autor:
Levy, Rebecca C., Bolatto, Alberto D., Leroy, Adam K., Sormani, Mattia C., Emig, Kimberly L., Gorski, Mark, Lenkić, Laura, Mills, Elisabeth A. C., Tarantino, Elizabeth, Teuben, Peter, Veilleux, Sylvain, Walter, Fabian
The center of the nearby galaxy NGC\,253 hosts a population of more than a dozen super star clusters (SSCs) which are still in the process of forming. The majority of the star formation of the burst is concentrated in these SSCs, and the starburst is
Externí odkaz:
http://arxiv.org/abs/2206.04700