Zobrazeno 1 - 10
of 118
pro vyhledávání: '"van der Hulst, Thijs"'
Autor:
Conrado, Ana M., Delgado, Rosa M. González, García-Benito, Rubén, Pérez, Isabel, Verley, Simon, Ruiz-Lara, Tomás, Sánchez-Menguiano, Laura, Puertas, Salvador Duarte, Jiménez, Andoni, Domínguez-Gómez, Jesús, Espada, Daniel, Argudo-Fernández, María, Alcázar-Laynez, Manuel, Blázquez-Calero, Guillermo, Bidaran, Bahar, Zurita, Almudena, Peletier, Reynier, Torres-Ríos, Gloria, Florido, Estrella, Martínez, Mónica Rodríguez, del Moral-Castro, Ignacio, van de Weygaert, Rien, Falcón-Barroso, Jesús, Lugo-Aranda, Alejandra Z., Sánchez, Sebastián F., van der Hulst, Thijs, Courtois, Hélène M., Ferré-Mateu, Anna, Sánchez-Blázquez, Patricia, Román, Javier, Aceituno, Jesús
Publikováno v:
A&A 687, A98 (2024)
The Universe is shaped as a web-like structure, formed by clusters, filaments, and walls that leave large volumes in between named voids. Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution tha
Externí odkaz:
http://arxiv.org/abs/2404.10823
Autor:
Domínguez-Gómez, Jesús, Pérez, Isabel, Ruiz-Lara, Tomás, Peletier, Reynier F., Sánchez-Blázquez, Patricia, Lisenfeld, Ute, Bidaran, Bahar, Falcón-Barroso, Jesús, Alcázar-Laynez, Manuel, Argudo-Fernández, María, Blázquez-Calero, Guillermo, Courtois, Hélène, Puertas, Salvador Duarte, Espada, Daniel, Florido, Estrella, García-Benito, Rubén, Jiménez, Andoni, Kreckel, Kathryn, Relaño, Mónica, Sánchez-Menguiano, Laura, van der Hulst, Thijs, van de Weygaert, Rien, Verley, Simon, Zurita, Almudena
Publikováno v:
A&A 680, A111 (2023)
Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors than galaxies in denser environments, that is, in filaments, walls, and clusters. The stellar metallic
Externí odkaz:
http://arxiv.org/abs/2310.11412
Autor:
Namumba, Brenda, Román, Javier, Barroso, Jesus Falcon, Knapen, Johan H., Roger, Ianjamasimanana, Naluminsa, Elizabeth, Jozsa, Gyula I. G., Korsaga, Marie, Maddox, Natasha, Frank, Brad, Sikhosana, Sinenhlanhla, Legodi, Samuel, Carignan, Claude, Ponomareva, Anastasia A., Jarrett, Tom, Lucero, Danielle, Smirnov, Oleg M., van der Hulst, Thijs, Pisano, D. J., Malek, kasia, Marchetti, Lucia, Vaccari, Mattia, Jarvis, Matt, Baes, Maarten, Meyer, Martin, Adams, Elizabeth A. K., Delhaize, Jacinta, Chen, Hao, Rajohnson, Sambatriniaina, Kurapati, Sushma, Heywood, Ian, Verdes-Montenegro, Lourdes
The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (\HI) is an excellent way to trace these interactions. Here, we present \HI\ observations of the spiral galaxy NGC~895, which w
Externí odkaz:
http://arxiv.org/abs/2303.09371
Autor:
Gogate, Avanti, Verheijen, Marc, Deshev, Boris, Montero-Castaño, Maria, van Gorkom, Jacqueline, van der Hulst, Thijs, Jaffé, Yara, Poggianti, Bianca
Publikováno v:
2020MNRAS.496.3531G
In this paper, we present data from the Blind Ultra-Deep HI Environmental Survey (BUDHIES), which is a blind 21-cm HI spectral line imaging survey undertaken with the Westerbork Synthesis Radio Telescope (WSRT). Two volumes were surveyed, each with a
Externí odkaz:
http://arxiv.org/abs/2302.12197
Autor:
Pan, Hengxing, Jarvis, Matt J., Santos, Mario G., Maddox, Natasha, Frank, Bradley S., Ponomareva, Anastasia A., Prandoni, Isabella, Kurapati, Sushma, Baes, Maarten, Piña, Pavel E. Mancera, Rodighiero, Giulia, Meyer, Martin J., Davé, Romeel, Sharma, Gauri, Rajohnson, Sambatriniaina H. A., Adams, Nathan J., Bowler, Rebecca A. A., Sinigaglia, Francesco, van der Hulst, Thijs, Hatfield, Peter W., Sekhar, Srikrishna, Collier, Jordan D.
We study the $M_{\rm HI}-M_{\star}$ relation over the last billion years using the MIGHTEE-HI sample. We first model the upper envelope of the $M_{\rm HI}-M_{\star}$ relation with a Bayesian technique applied to a total number of 249 HI-selected gala
Externí odkaz:
http://arxiv.org/abs/2210.04651
Autor:
van Leeuwen, Joeri, Kooistra, Eric, Oostrum, Leon, Connor, Liam, Hargreaves, J. E., Maan, Yogesh, Pastor-Marazuela, Inés, Petroff, Emily, van der Schuur, Daniel, Sclocco, Alessio, Straal, Samayra M., Vohl, Dany, Wijnholds, Stefan J., Adams, Elizabeth A. K., Adebahr, Björn, Attema, Jisk, Bassa, Cees, Bast, Jeanette E., Bilous, Anna, de Blok, W. J. G., Boersma, Oliver M., van Cappellen, Wim A., Coolen, Arthur H. W. M., Damstra, Sieds, Dénes, Helga, van Diepen, Ger N. J., Gardenier, David W., Grange, Yan G., Gunst, André W., Hess, Kelley M., Holties, Hanno, van der Hulst, Thijs, Hut, Boudewijn, Kutkin, Alexander, Loose, G. Marcel, Lucero, Danielle M., Mika, Ágnes, Mikhailov, Klim, Morganti, Raffaella, Moss, Vanessa A., Mulder, Henk, Norden, Menno J., Oosterloo, Tom A., Orrú, Emaneula, Paragi, Zsolt, de Reijer, Jan-Pieter R., Schoenmakers, Arno P., Stuurwold, Klaas J. C., ter Veen, Sander, Wang, Yu-Yang, Zanting, Alwin W., Ziemke, Jacob
Publikováno v:
A&A 672, A117 (2023)
Fast Radio Bursts must be powered by uniquely energetic emission mechanisms. This requirement has eliminated a number of possible source types, but several remain. Identifying the physical nature of Fast Radio Burst (FRB) emitters arguably requires g
Externí odkaz:
http://arxiv.org/abs/2205.12362
Autor:
Morganti, Raffaella, Jurlin, Nika, Oosterloo, Tom, Brienza, Marisa, Orru', Emanuela, Kutkin, Alexander, Prandoni, Isabella, Adams, Elizabeth A. K., Denes, Helga, Hess, Kelley M., Shulevski, Aleksandar, van der Hulst, Thijs, Ziemke, Jacob
Active galactic nuclei (AGN) at the centres of galaxies can cycle between periods of activity and of quiescence. Characterising the duty-cycle of AGN is crucial for understanding their impact on the evolution of the host galaxy. For radio AGN, their
Externí odkaz:
http://arxiv.org/abs/2111.04776
Autor:
Pastor-Marazuela, Inés, Connor, Liam, van Leeuwen, Joeri, Maan, Yogesh, ter Veen, Sander, Bilous, Anna, Oostrum, Leon, Petroff, Emily, Straal, Samayra, Vohl, Dany, Attema, Jisk, Boersma, Oliver M., Kooistra, Eric, van der Schuur, Daniel, Sclocco, Alessio, Smits, Roy, Adams, Elizabeth A. K., Adebahr, Björn, de Blok, Willem J. G., Coolen, Arthur H. W. M., Damstra, Sieds, Dénes, Helga, Hess, Kelley M., van der Hulst, Thijs, Hut, Boudewijn, Ivashina, V. Marianna, Kutkin, Alexander, Loose, G. Marcel, Lucero, Danielle M., Mika, Ágnes, Moss, Vanessa A., Mulder, Henk, Norden, Menno J., Oosterloo, Tom, Orrú, Emanuela, Ruiter, Mark, Wijnholds, Stefan J.
Fast radio bursts (FRBs) are extragalactic astrophysical transients whose brightness requires emitters that are highly energetic, yet compact enough to produce the short, millisecond-duration bursts. FRBs have thus far been detected between 300 MHz a
Externí odkaz:
http://arxiv.org/abs/2012.08348
Autor:
Wang, Jing, Koribalski, Baerbel S., Jarrett, Tom H., Kamphuis, Peter, Li, Zhao-Yu, Ho, Luis C., Westmeier, Tobias, Shao, Li, Lagos, Claudia del P., Wong, O. Ivy, Serra, Paolo, Staveley-Smith, Lister, Jozsa, Gyula, van der Hulst, Thijs, Lopez-Sanchez, A. R.
We built a multi-wavelength dataset for galaxies from the Local Volume HI Survey (LVHIS), which comprises 82 galaxies. We also select a sub-sample of ten large galaxies for investigating properties in the galactic outskirts. The LVHIS sample covers n
Externí odkaz:
http://arxiv.org/abs/1708.02744
Asymmetries in the neutral hydrogen gas distribution and kinematics of galaxies are thought to be indicators for both gas accretion and gas removal processes. These are of fundamental importance for galaxy formation and evolution. Upcoming large blin
Externí odkaz:
http://arxiv.org/abs/1606.07387