Search Results - "Di Mille, Francesco"

Raman-scattered O vi Features in the Symbiotic Nova RR Telescopii by Heo, Jeong-Eun, Lee, Hee-Won, Angeloni, Rodolfo, Palma, Tali, Mille, Francesco Di

“…Abstract RR Telescopii (RR Tel) is an interacting binary system in which a hot white dwarf (WD) accretes matter from a Mira-type variable star via…”
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A PROFILE ANALYSIS OF RAMAN-SCATTERED O VI BANDS AT 6825 AND 7082 IN SANDULEAK'S STAR by Heo, Jeong-Eun, Angeloni, Rodolfo, Mille, Francesco Di, Palma, Tali, Lee, Hee-Won

“…ABSTRACT We present a detailed modeling of the two broad bands observed at 6825 and 7082 in Sanduleak's star, a controversial object in the Large Magellanic…”
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FORMATION OF RAMAN SCATTERING WINGS AROUND H α , H β , AND PA α IN ACTIVE GALACTIC NUCLEI by Chang, Seok-Jun, Heo, Jeong-Eun, Mille, Francesco Di, Angeloni, Rodolfo, Palma, Tali, Lee, Hee-Won

“…Powered by a supermassive black hole with an accretion disk, the spectra of active galactic nuclei (AGNs) are characterized by prominent emission lines…”
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Extended Narrow-Line Region in Seyfert Galaxies by Congiu, Enrico, Contini, Marcella, Ciroi, Stefano, Cracco, Valentina, Di Mille, Francesco, Berton, Marco, Frezzato, Michele, La Mura, Giovanni, Rafanelli, Piero

“…We present our recent results about the extended narrow-line region (ENLR) of two nearby Seyfert 2 galaxies (IC 5063 and NGC 7212) obtained by modeling the…”
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Raman-scattered O VI features in the symbiotic nova RR Telescopii by Heo, Jeong-Eun, Lee, Hee-Won, Angeloni, Rodolfo, Palma, Tali, Di Mille, Francesco

“…RR Tel is an interacting binary system in which a hot white dwarf (WD) accretes matter from a Mira-type variable star via gravitational capture of its stellar…”
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SDSS J211852.96-073227.5: The first non-local, interacting, late-type intermediate Seyfert galaxy with relativistic jets by Järvelä, Emilia, Berton, Marco, Ciroi, Stefano, Congiu, Enrico, Lähteenmäki, Anne, Di Mille, Francesco

“…A&A 636, L12 (2020) It has been often suggested that a tangible relation exists between relativistic jets in active galactic nuclei (AGN) and the morphology of…”
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X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6.56 by Wolf, Julien, Nandra, Kirpal, Salvato, Mara, Buchner, Johannes, Onoue, Masafusa, Liu, Teng, Arcodia, Riccardo, Merloni, Andrea, Ciroi, Stefano, Di Mille, Francesco, Burwitz, Vadim, Brusa, Marcella, Ishimoto, Rikako, Kashikawa, Nobunari, Matsuoka, Yoshiki, Urrutia, Tanya, Waddell, Sophia

“…A&A 669, A127 (2023) This study aims at identifying luminous quasars at $z>5.7$ among X-ray-selected sources in the eROSITA Final Equatorial-Depth Survey…”
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A Profile Analysis of Raman-scattered O VI Bands at 6825 \AA\ and 7082 \AA\ in Sanduleak's Star by Heo, Jeong-Eun, Angeloni, Rodolfo, Di Mille, Francesco, Palma, Tali, Lee, Hee-Won

“…We present a detailed modeling of the two broad bands observed at 6825 \AA\ and 7082 \AA\ in Sanduleak's star, a controversial object in the Large Magellanic…”
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Blue large-amplitude pulsators as a new class of variable stars by Pietrukowicz, Paweł, Dziembowski, Wojciech A., Latour, Marilyn, Angeloni, Rodolfo, Poleski, Radosław, di Mille, Francesco, Soszyński, Igor, Udalski, Andrzej, Szymański, Michał K., Wyrzykowski, Łukasz, Kozłowski, Szymon, Skowron, Jan, Skowron, Dorota, Mróz, Przemek, Pawlak, Michał, Ulaczyk, Krzysztof

“…Regular intrinsic brightness variations observed in many stars are caused by pulsations. These pulsations provide information on the global and structural…”
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A Census of the Supersoft X-ray Sources in M31 by Orio, Marina, Nelson, Thomas, Bianchini, Antonio, Di Mille, Francesco, Harbeck, Daniel

“…We examined X-ray, ultraviolet, and optical archival data of 89 supersoft X-ray sources (SSS) in M31. We studied the timescales of X-ray variability and…”
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FORMATION OF RAMAN SCATTERING WINGS AROUND H[alpha], H[beta], AND PA[alpha] IN ACTIVE GALACTIC NUCLEI by Chang, Seok-Jun, Heo, Jeong-Eun, Mille, Francesco Di, Angeloni, Rodolfo, Palma, Tali, Lee, Hee-Won

“…Powered by a supermassive black hole with an accretion disk, the spectra of active galactic nuclei (AGNs) are characterized by prominent emission lines…”
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FORMATION OF RAMAN SCATTERING WINGS AROUND H , Hβ, AND PA IN ACTIVE GALACTIC NUCLEI by Chang, Seok-Jun, Heo, Jeong-Eun, Mille, Francesco Di, Angeloni, Rodolfo, Palma, Tali, Lee, Hee-Won

“…ABSTRACT Powered by a supermassive black hole with an accretion disk, the spectra of active galactic nuclei (AGNs) are characterized by prominent emission…”
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X-RAY GRATING OBSERVATIONS OF RECURRENT NOVA T PYXIDIS DURING THE 2011 OUTBURST by TOFFLEMIRE, BENJAMIN M, Orio, Marina, Page, Kim L, Osborne, Julian P, Ciroi, Stefano, Cracco, Valentina, Di Mille, Francesco, Maxwell, Michael

“…The recurrent nova T Pyx was observed with the X-ray gratings of Chandra and XMM-Newton, 210 and 235 days, respectively, after the discovery of the 2011 April…”
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Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger by Kilpatrick, Charles D, Foley, Ryan J, Kasen, Daniel, Murguia-Berthier, Ariadna, Ramirez-Ruiz, Enrico, Coulter, David A, Drout, Maria R, Piro, Anthony L, Shappee, Benjamin J, Boutsia, Konstantina, Contreras, Carlos, Di Mille, Francesco, Madore, Barry F, Morrell, Nidia, Pan, Yen-Chen, Prochaska, J. Xavier, Rest, Armin, Rojas-Bravo, César, Siebert, Matthew R, Simon, Joshua D, Ulloa, Natalie

“…11 hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an…”
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X-Ray Grating Observations of Recurrent Nova T Pyxidis During The 2011 Outburst by Tofflemire, Benjamin M, Orio, Marina, Page, Kim L, Osborne, Julian P, Ciroi, Stefano, Cracco, Valentina, Di Mille, Francesco, Maxwell, Michael

“…The recurrent nova T Pyx was observed with the X-ray gratings of Chandra and XMM-Newton, 210 and 235 days, respectively, after the discovery of the 2011 April…”
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On the nature of CP Pup by Mason, Elena, Orio, Marina, Mukai, Koji, Bianchini, Antonio, de Martino, Domitilla, di Mille, Francesco, Williams, Robert E, Abbot, Timothy, de Propris, Roberto

“…We present new X-ray and optical spectra of the old nova CP Pup (nova Pup 1942) obtained with Chandra and the CTIO 4m telescope. The X-ray spectrum reveals a…”
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Escape of Resonantly Scattered Ly$\beta$ and H$\alpha$ from Hot and Optically Thick Media by Chang, Seok-Jun, Lee, Hee-Won, Ahn, Sang-Hyeon, Lee, Hogyu, Angeloni, Rodolfo, Palma, Tali, Di Mille, Francesco

“…We investigate the escape of Ly$\beta$ from emission nebulae with a significant population of excited hydrogen atoms in the level $n=2$, rendering them…”
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Extended narrow-line region in Seyfert galaxies by Congiu, Enrico, Contini, Marcella, Ciroi, Stefano, Cracco, Valentina, Di Mille, Francesco, Berton, Marco, Frezzato, Michele, La Mura, Giovanni, Rafanelli, Piero, .

“…We present our recent results about the extended narrow-line region (ENLR) of two nearby Seyfert 2 galaxies (IC 5063 and NGC 7212) obtained by modelling the…”
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Formation of Raman Scattering Wings around H alpha, H beta and Pa alpha in Active Galactic Nuclei by Chang, Seok-Jun, Heo, Jeong-Eun, Di Mille, Francesco, Angeloni, Rodolfo, Palma, Tali, Lee, Hee-Won

“…Powered by a supermassive black hole with an accretion disk, the spectra of active galactic nuclei (AGNs) are characterized by prominent emission lines…”
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The multiple periods and the magnetic nature of CP Pup by Mason, Elena, Bianchini, Antonio, Orio, Marina, Williams, Robert E, Mukai, Koji, de Marino, Domitilla, Abbot, Timothy . M. C, di Mille, Francesco

“…Fast cadence time resolved spectra taken at the CTIO-4m telescope with the RC-spectrograph during 2 consecutive nights revealed a long term modulation of the…”
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