Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Archana Aravindan"'
Publikováno v:
The Astrophysical Journal, Vol 975, Iss 1, p 60 (2024)
Detecting active black holes in dwarf galaxies has proven to be a challenge due to their small size and weak electromagnetic signatures. Mid-infrared variability has emerged as a promising tool that can be used to detect active low-mass black holes i
Externí odkaz:
https://doaj.org/article/4b650dfafcd74a4f9f92b1675f48751e
Autor:
Weizhe Liu, Sylvain Veilleux, Gabriela Canalizo, Todd M. Tripp, David S. N. Rupke, Archana Aravindan, Thomas Bohn, Fred Hamann, Christina M. Manzano-King
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 152 (2024)
While stellar processes are believed to be the main source of feedback in dwarf galaxies, the accumulating discoveries of active galactic nuclei (AGN) in dwarf galaxies over recent years arouse the interest to also consider AGN feedback in them. Fast
Externí odkaz:
https://doaj.org/article/15f09f2fe50f4927b8811ad1dabafb78
Autor:
Michael Reefe, Shobita Satyapal, Remington O. Sexton, Nathan J. Secrest, William Matzko, Emma Schwartzman, Kristina Nyland, Gabriela Canalizo, Barry Rothberg, Ryan W. Pfeifle, Jenna M. Cann, Archana Aravindan, Camilo Vazquez, Tracy Clarke
Publikováno v:
The Astrophysical Journal Letters, Vol 946, Iss 2, p L38 (2023)
Local low-metallicity dwarf galaxies are relics of the early universe and are thought to hold clues into the origins of supermassive black holes. While recent studies are uncovering a growing population of active galactic nuclei (AGNs) in dwarf galax
Externí odkaz:
https://doaj.org/article/5956c4b9fab04ade95e51c4b43888731
Autor:
Archana Aravindan, Weizhe Liu, Gabriela Canalizo, Sylvain Veilleux, Thomas Bohn, Remington O. Sexton, David S. N. Rupke, Vivian U
Publikováno v:
The Astrophysical Journal, Vol 950, Iss 1, p 33 (2023)
Feedback likely plays a crucial role in resolving discrepancies between observations and theoretical predictions of dwarf galaxy properties. Stellar feedback was once believed to be sufficient to explain these discrepancies, but it has thus far faile
Externí odkaz:
https://doaj.org/article/74aa119e13954ac9b03fd54afc02a32f
Autor:
Michael Reefe, Shobita Satyapal, Remington O. Sexton, Nathan J. Secrest, William Matzko, Emma Schwartzman, Kristina Nyland, Gabriela Canalizo, Barry Rothberg, Ryan W. Pfeifle, Jenna M. Cann, Archana Aravindan, Camilo Vazquez, Tracy Clarke
Local low metallicity dwarf galaxies are relics of the early universe and hold clues into the origins of supermassive black holes (SMBHs). In recent work, coronal lines have been used to unveil a population of candidate accreting black holes in dwarf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::722bd8cd6d6d2ee54fc420faf2db6c43
http://arxiv.org/abs/2211.13179
http://arxiv.org/abs/2211.13179
Publikováno v:
International Journal of Management Studies. :10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eaf024bc9755ae7c3ab66bdf20361a61
https://doi.org/10.18843/ijms/v5is1/02
https://doi.org/10.18843/ijms/v5is1/02