Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Bhowmik, Trisha"'
Autor:
Kaur, Simranpreet, Girart, Josep M., Viganò, Daniele, Monge, Álvaro Sánchez, Cleeves, L. Ilsedore, Zurlo, Alice, Del Sordo, Fabio, Morata, Òscar, Bhowmik, Trisha, Alves, Felipe O.
The young stellar object [BHB2007]-1 has been extensively studied in the past at radio, millimeter, and infrared wavelengths. It shows a gap in the disk and previous observations claimed the possible emission from a forming sub-stellar object, in cor
Externí odkaz:
http://arxiv.org/abs/2408.04025
Autor:
Casassus, Simon, Cieza, Lucas, Cárcamo, Miguel, Ribas, Álvaro, Christiaens, Valentin, Rodríguez-Jiménez, Abigali, Arce-Tord, Carla, Bhowmik, Trisha, Chavan, Prachi, González-Ruilova, Camilo, Martínez-Brunner, Rafael, Guidotti, Valeria, Leiva, Mauricio
Environmental effects, such as stellar fly-bys and external irradiation, are thought to affect the evolution of protoplanetary disks in clustered star formation. Previous ALMA images at 225 GHz of the ISO-Oph 2 binary revealed a peculiar morphology i
Externí odkaz:
http://arxiv.org/abs/2307.07416
Autor:
Nogueira, Pedro Henrique, Zurlo, Alice, Pérez, Sebastián, González-Ruilova, Camilo, Cieza, Lucas A., Hales, Antonio, Bhowmik, Trisha, Ruíz-Rodríguez, Dary A., Principe, David A., Herczeg, Gregory J., Williams, Jonathan P., Cuadra, Jorge, Montesinos, Matías, Cuello, Nicolás, Chavan, Prachi, Casassus, Simon, Zhu, Zhaohuan, Goicovic, Felipe G.
Episodic accretion is a low-mass pre-main sequence phenomenon characterized by sudden outbursts of enhanced accretion. These objects are classified into two: protostars with elevated levels of accretion that lasts for decades or more, called FUors, a
Externí odkaz:
http://arxiv.org/abs/2305.15647
Autor:
Singh, Garima, Bhowmik, Trisha, Boccaletti, Anthony, Thébault, Philippe, Kral, Quentin, Milli, Julien, Mazoyer, Johan, Pantin, Eric, Olofsson, Johan, Boukrouche, Ryan, Di Folco, Emmanuel, Janson, Markus, Langlois, Maud, Maire, Anne Lise, Vigan, Arthur, Benisty, Myriam, Augereau, Jean-Charles, Perrot, Clement, Gratton, Raffaele, Henning, Thomas, Ménard, Francois, Rickman, Emily, Wahhaj, Zahed, Zurlo, Alice, Biller, Beth, Bonnefoy, Mickael, Chauvin, Gael, Delorme, Philippe, Desidera, Silvano, D'Orazi, Valentina, Feldt, Markus, Hagelberg, Janis, Keppler, Miriam, Kopytova, Taisiya, Lagadec, Eric, Lagrange, Anne-Marie, Mesa, Dino, Meyer, Michael, Rouan, Daniel, Sissa, Elena, Schmidt, Tobias, Jaquet, Marc, Fusco, Thierry, Pavlov, Alexei, Rabou, Patrick
Publikováno v:
A&A 653, A79 (2021)
We obtained polarimetric differential imaging of a gas-rich debris disk around HD 141569A with SPHERE in the H-band to compare the scattering properties of the innermost ring at 44 au with former observations in total intensity with the same instrume
Externí odkaz:
http://arxiv.org/abs/2107.07570
Akademický článek
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Autor:
Nowak, Mathias, Rajkumar, Anitha Raj, Oliveros Gomez, Natalia, Bhowmik, Trisha, Mysore, Harshitha, Medina, Sofia
The presentation begins by describing how to download the VLTI-GRAVITY instrument's archival data (2018-09-21). The EsoReflex environment is used to carry out the data reduction steps. To understand the astrometry and spectrum of Beta Pic b, two pipe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::669c6ea5f52ff1ee6cd4eef4f68ee834
Autor:
Novak, Mathais, Parashivamurthy, Harshitha Mysore, Bhowmik, Trisha, Rajkumar, Anitha Raj, Oliveros Gomez, Natalia, Medina, Sofia
This is the final presentation and a summary of the work we did during the VLTI-HOW workshop under Mathais Novak, University of Cambridge. The data from the night of September 21, 2018 of the system beta pic b obtained from the GRAVITY-VLTI instrumen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9b23a4f243fcee6c3aa7b4bfe221af73
Publikováno v:
Journal of Complementary & Integrative Medicine; Mar2023, Vol. 20 Issue 1, p47-80, 34p
Autor:
Bhowmik, Trisha
Publikováno v:
Astrophysics [astro-ph]. Université Paris sciences et lettres, 2019. English. ⟨NNT : 2019PSLEO019⟩
Debris disks are found around many young main-sequence stars. They are characterized by the dusty, gas-depleted environment as opposed to gas-rich protoplanetary disks. Debris disks are also considered as `secondary disks' because they bear non-primo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::21330377ace7ebb39061dd49724d91d5
Autor:
Bhowmik, Trisha
Publikováno v:
Astrophysics [astro-ph]. Université Paris sciences et lettres, 2019. English. ⟨NNT : 2019PSLEO019⟩
Debris disks are found around many young main-sequence stars. They are characterized by the dusty, gas-depleted environment as opposed to gas-rich protoplanetary disks. Debris disks are also considered as `secondary disks' because they bear non-primo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______212::b545ab73f4ef11ece234c3a9da4c43ba
https://tel.archives-ouvertes.fr/tel-02966928
https://tel.archives-ouvertes.fr/tel-02966928