Search Results - "Kirsanova, Maria S."

3D structure of H ii regions in the star-forming complex S254-S258 by Kirsanova, Maria S, Moiseev, Alexei V, Boley, Paul A

“…ABSTRACT The S254-258 star-forming complex is a place of massive star formation where five OB-stars have created H ii regions, visible as optical nebulae, and…”
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Merged H/H2 and C+/C/CO transitions in the Orion Bar by Kirsanova, Maria S, Wiebe, Dmitri S

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Orion Bar as a window to the evolution of PAHs by Murga, Maria S, Kirsanova, Maria S, Wiebe, Dmitry S, Boley, Paul A

“…ABSTRACT We investigate the mid-infrared (IR) emission in the Orion Bar photodissociation region (PDR), using archival photometric and spectroscopic…”
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Dark cloud-type chemistry in photodissociation regions with moderate ultraviolet field by Kirsanova, Maria S, Punanova, Anna F, Semenov, Dmitry A, Vasyunin, Anton I

“…ABSTRACT We present a study of emission lines of small hydrocarbons C2H and c-C3H2, and COMs precursors H2CO and CH3OH in order to better understand the…”
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NH3 observations of the S235 star-forming region: Dense gas in inter-core bridges by Burns, Ross A, Handa, Toshihiro, Omodaka, Toshihiro, Sobolev, Andrej M, Kirsanova, Maria S, Nagayama, Takumi, Chibueze, James O, Kohno, Mikito, Nakano, Makoto, Sunada, Kazuyoshi, Ladeyschikov, Dmitry A

“…Abstract Star formation is thought to be driven by two groups of mechanisms; spontaneous collapse and triggered collapse. Triggered star formation mechanisms…”
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Molecular gas in high-mass filament WB673 by Kirsanova, Maria S., Salii, Svetlana V., Sobolev, Andrej M., Olofsson, Anders Olof Henrik, Ladeyschikov, Dmitry A., Thomasson, Magnus

“…We studied the distribution of dense gas in a filamentary molecular cloud containing several dense clumps. The center of the filament is given by the dense…”
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Ethynyl around the HII regions S255 and S257 by Buslaeva, Anna I, Kirsanova, Maria. S, Punanova, Anna F

“…We present the results of the ethynyl (C2H) emission line observations towards the HII regions S255 and S257 and the molecular cloud between them. Radial…”
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PDRs4All: A JWST Early Release Science Program on Radiative Feedback from Massive Stars by Berné, Olivier, Habart, Émilie, Abergel, Alain, Bernard-Salas, Jeronimo, Bron, Emeric, Dartois, Emmanuel, Fuente, Asunción, Okada, Yoko, Onaka, Takashi, Tielens, Alexander G. G. M., Vicente, Sílvia, Wolfire, Mark G., Alarcón, Felipe, Boersma, C., Canin, Amélie, Chown, Ryan, Dicken, Daniel, Le Gal, Romane, Trahin, Boris, Simmer, Thomas, Van De Putte, Dries, Cuadrado, Sara, Maragkoudakis, Alexandros, Schefter, Bethany R., Schirmer, Thiébaut, Cazaux, Stéphanie, Aleman, Isabel, Allamandola, Louis, Antonio Baratta, Giuseppe, Bejaoui, Salma, Bera, Partha P., Black, John H., Boulanger, Francois, Brechignac, Philippe, Brünken, Sandra, Burkhardt, Andrew, Candian, Alessandra, Chabot, Marin, Chakraborty, Shubhadip, Cooke, Ilsa R., Coutens, Audrey, Demyk, Karine, Donovan Meyer, Jennifer, Engrand, Cécile, Foschino, Sacha, García-Lario, Pedro, Guillard, Pierre, Gusdorf, Antoine, Hartigan, Patrick, He, Jinhua, Herbst, Eric, Hornekaer, Liv, Jäger, Cornelia, Janot-Pacheco, Eduardo, Kaufman, Michael, Kendrew, Sarah, Kirsanova, Maria S., Klaassen, Pamela, Knight, Collin, Labiano, Álvaro, Lee, Timothy J., Lefloch, Bertrand, Le Petit, Franck, Linz, Hendrik, Mackie, Cameron J., Madden, Suzanne C., McGuire, Brett A., Micelotta, Elisabetta R., Misselt, Karl, Mulas, Giacomo, Neelamkodan, Naslim, Omont, Alain, Paladini, Roberta, Elisabetta Palumbo, Maria, Pathak, Amit, Pendleton, Yvonne J., Petrignani, Annemieke, Rangwala, Naseem, Rapacioli, Mathias, Ricca, Alessandra, Roman-Duval, Julia, Roser, Joseph, Roueff, Evelyne, Rouillé, Gaël, Salama, Farid, Sales, Dinalva A., Sandstrom, Karin, Sarre, Peter, Sellgren, Kris, Shannon, Matthew J., Shenoy, Sachindev S., Teyssier, David, Thomas, Richard D., Togi, Aditya, Witt, Adolf N., Wootten, Alwyn, Zettergren, Henning, Zhang, Yong, Zhang, Ziwei E., Zhen, Junfeng

“…Abstract Massive stars disrupt their natal molecular cloud material through radiative and mechanical feedback processes. These processes have profound effects…”
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A far-ultraviolet-driven photoevaporation flow observed in a protoplanetary disk by Berné, Olivier, Habart, Emilie, Peeters, Els, Schroetter, Ilane, Canin, Amélie, Sidhu, Ameek, Chown, Ryan, Bron, Emeric, Haworth, Thomas J, Klaassen, Pamela, Trahin, Boris, Van De Putte, Dries, Alarcón, Felipe, Zannese, Marion, Abergel, Alain, Bergin, Edwin A, Bernard-Salas, Jeronimo, Boersma, Christiaan, Cami, Jan, Cuadrado, Sara, Dartois, Emmanuel, Dicken, Daniel, Elyajouri, Meriem, Fuente, Asunción, Goicoechea, Javier R, Gordon, Karl D, Issa, Lina, Joblin, Christine, Kannavou, Olga, Khan, Baria, Lacinbala, Ozan, Languignon, David, Le Gal, Romane, Maragkoudakis, Alexandros, Meshaka, Raphael, Okada, Yoko, Onaka, Takashi, Pasquini, Sofia, Pound, Marc W, Robberto, Massimo, Röllig, Markus, Schefter, Bethany, Schirmer, Thiébaut, Simmer, Thomas, Tabone, Benoit, Tielens, Alexander G G M, Vicente, Sílvia, Wolfire, Mark G, Aleman, Isabel, Allamandola, Louis, Auchettl, Rebecca, Baratta, Giuseppe Antonio, Baruteau, Clément, Bejaoui, Salma, Bera, Partha P, Black, John H, Boulanger, Francois, Bouwman, Jordy, Brandl, Bernhard, Brechignac, Philippe, Brünken, Sandra, Buragohain, Mridusmita, Burkhardt, Andrew, Candian, Alessandra, Cazaux, Stéphanie, Cernicharo, Jose, Chabot, Marin, Chakraborty, Shubhadip, Champion, Jason, Colgan, Sean W J, Cooke, Ilsa R, Coutens, Audrey, Cox, Nick L J, Demyk, Karine, Meyer, Jennifer Donovan, Engrand, Cécile, Foschino, Sacha, García-Lario, Pedro, Gavilan, Lisseth, Gerin, Maryvonne, Godard, Marie, Gottlieb, Carl A, Guillard, Pierre, Gusdorf, Antoine, Hartigan, Patrick, He, Jinhua, Herbst, Eric, Hornekaer, Liv, Jäger, Cornelia, Janot-Pacheco, Eduardo, Kaufman, Michael, Kemper, Francisca, Kendrew, Sarah, Kirsanova, Maria S, Knight, Collin, Kwok, Sun, Labiano, Álvaro, Lai, Thomas S-Y, Lee, Timothy J, Lefloch, Bertrand

“…Most low-mass stars form in stellar clusters that also contain massive stars, which are sources of far-ultraviolet (FUV) radiation. Theoretical models predict…”
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Molecular gas in high-mass filament WB 673 by Kirsanova, M. S., Salii, Svetlana V., Sobolev, A. M., Olofsson, Henrik, Ladeyschikov, Dmitry A., Thomasson, Magnus

“…We studied the distribution of dense gas in a filamentary molecular cloud containing several dense clumps. The center of the filament is given by the dense…”
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Infrared appearance of wind-blown bubbles around young massive stars by Kirsanova, Maria S, Pavlyuchenkov, Yaroslav N

“…Thousands of ring-like bubbles appear on infrared images of the Galaxy plane. Most of these infrared bubbles form during expansion of HII regions around…”
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3D structure of HII regions in the star-forming complex S254-S258 by Kirsanova, Maria S, Moiseev, Alexei V, Boley, Paul A

“…The S254-258 star-forming complex is a place of massive star formation where five OB-stars have created HII regions, visible as optical nebulae, and disrupted…”
Get full text

Merged H/H2 and C+/C/CO transitions in the Orion Bar by Kirsanova, Maria S, Wiebe, Dmitri S

“…High-resolution ALMA images towards the Orion Bar show no discernible offset between the peak of H2 emission in the photodissociation region (PDR) and the…”
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Orion Bar as a window to the evolution of PAHs by Murga, Maria S, Kirsanova, Maria S, Wiebe, Dmitry S, Boley, Paul A

“…MNRAS, 509, 800 (2022) We investigate the mid-infrared (IR) emission in the Orion Bar photodissociation region, using archival photometric and spectroscopic…”
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Dark cloud-type chemistry in PDRs with moderate UV field by Kirsanova, Maria S, Punanova, Anna F, Semenov, Dmitry A, Vasyunin, Anton I

“…We present a study of emission lines of small hydrocarbons C$_2$H and $c$-C$_3$H$_2$, and COMs precursors H$_2$CO and CH$_3$OH in order to better understand…”
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Global photometric analysis of galactic HII regions by Topchieva, Anastasiia, Wiebe, Dmitri, Kirsanova, Maria S

“…Total infrared fluxes are estimated for 99 HII regions around massive stars. The following wavebands have been used for the analysis: 8 and 24 $\mu$m, based on…”
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NH$_3$ Observations of the S235 Star Forming Region: Dense Gas in Inter-core Bridges by Burns, Ross A, Handa, Toshihiro, Omodaka, Toshihiro, Sobolev, Andrej M, Kirsanova, Maria S, Nagayama, Takumi, Chibueze, James O, Kohno, Mikito, Nakano, Makoto, Sunada, Kazuyoshi, Ladeyschikov, Dmitry A

“…Star formation is thought to be driven by two groups of mechanisms; spontaneous collapse and triggered collapse. Triggered star formation mechanisms further…”
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Physical conditions in star forming regions around S235 by Kirsanova, Maria S, Wiebe, Dmitry S, Sobolev, Andrej M, Henkel, Christian, Tsivilev, Alexander P

“…Gas density and temperature in star forming regions around Sh2-235 are derived from ammonia line observations. This information is used to evaluate formation…”
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