Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Amôres, Eduardo B."'
Autor:
Amores, Eduardo B., Jesus, Ricardo M., Moitinho, Andre, Arsenijevic, Vladan, Levenhagen, Ronaldo S., Marshall, Douglas J., Kerber, Leandro O., Kunzel, Roseli, Moura, Rodrigo A.
Estimates of interstellar extinction are essential in a broad range of astronomical research. In the last decades, several maps and models of the large scale interstellar extinction in the Galaxy have been published. However, these maps and models ha
Externí odkaz:
http://arxiv.org/abs/2108.00561
Autor:
Baravalle, Laura D., Alonso, M. Victoria, Minniti, Dante, Castellón, José Luis Nilo, Soto, Mario, Valotto, Carlos, Villalón, Carolina, Graña, Darío, Amôres, Eduardo B., Castro, F. Milla
Knowledge about the large-scale distribution of galaxies is far from complete in the Zone of Avoidance, which is mostly due to high interstellar extinction and to source confusion at lower Galactic latitudes. Past near-infrared (NIR) surveys, such as
Externí odkaz:
http://arxiv.org/abs/2012.14856
A study on the photosphere and disc of the Be star $\beta$ Psc is presented. We recover almost 40 years of high-resolution spectroscopic observations and additional data gathered from the BeSS database. We evaluate the photospheric parameters from th
Externí odkaz:
http://arxiv.org/abs/2009.06493
Autor:
Giribaldi, Riano E., de Mello, Gustavo F. Porto, Lorenzo-Oliveira, Diego, Amôres, Eduardo B., Ubaldo-Melo, Maria L.
Publikováno v:
A&A 629, A33 (2019)
The flux distribution of solar analogs is required for calculating the spectral albedo of Solar System bodies such as asteroids and trans-Neptunian objects. Ideally a solar analog should be comparably faint as the target of interest, but only few ana
Externí odkaz:
http://arxiv.org/abs/1907.00445
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Hempel, Maren, Minniti, Dante, Dékány, István, Saito, Roberto K., Lucas, Philip W., Emerson, Jim, Ahumada, Andrea V., Aigrain, Suzanne, Alonso, Maria Victoria, Alonso-García, Javier, Amôres, Eduardo B., Angeloni, Rodolfo, Arias, Julia, Bandyopadhyay, Reba, Barbá, Rodolfo H., Barbuy, Beatriz, Baume, Gustavo, Beamin, Juan Carlos, Bedin, Luigi, Bica, Eduardo, Borissova, Jordanka, Bronfman, Leonardo, Carraro, Giovanni, Catelan, Márcio, Clariá, Juan J., Contreras, Carlos, Cross, Nicholas, Davis, Christopher, de Grijs, Richard, Drew, Janet E., Fariña, Cecilia, Feinstein, Carlos, Lajús, Eduardo Fernández, Folkes, Stuart, Gamen, Roberto C., Geisler, Douglas, Gieren, Wolfgang, Goldman, Bertrand, González, Oscar, Gosling, Andrew, Gunthardt, Guillermo, Gurovich, Sebastian, Hambly, Nigel C., Hanson, Margaret, Hoare, Melvin, Irwin, Mike J., Ivanov, Valentin D., Jordán, Andrés, Kerins, Eamonn, Kinemuchi, Karen, Kurtev, Radostin, Longmore, Andy, López-Corredoira, Martin, Maccarone, Tom, Martín, Eduardo, Masetti, Nicola, Mennickent, Ronald E., Merlo, David, Messineo, Maria, Mirabel, I. Félix, Monaco, Lorenzo, Bidin, Christian Moni, Morelli, Lorenzo, Padilla, Nelson, Palma, Tali, Parisi, Maria Celeste, Parker, Quentin, Pavani, Daniela, Pietrukowicz, Pawel, Pietrzynski, Grzegorz, Pignata, Giuliano, Rejkuba, Marina, Rojas, Alejandra, Roman-Lopes, Alexandre, Ruiz, Maria Teresa, Sale, Stuart E., Saviane, Ivo, Schreiber, Matthias R., Schröder, Anja C., Sharma, Saurabh, Smith, Michael, Sodré Jr., Laerte, Soto, Mario, Stephens, Andrew W., Tamura, Motohide, Tappert, Claus, Thompson, Mark A., Toledo, Ignacio, Valenti, Elena, Vanzi, Leonardo, Weidmann, Walter, Zoccali, Manuela
Publikováno v:
ESO Messenger 155, (2014), 29-32
The VISTA Variables in the V\'ia L\'actea (VVV) survey is one of six public ESO surveys, and is now in its 4th year of observing. Although far from being complete, the VVV survey has already delivered many results, some directly connected to the inte
Externí odkaz:
http://arxiv.org/abs/1406.3241
We used the HI data from the LAB survey to map the ring-shaped gap in HI density which lies slightly outside the solar circle. Adopting $R_0$= 7.5 kpc, we find and average radius of 8.3 kpc and an average gap width of 0.8 kpc. The characteristics of
Externí odkaz:
http://arxiv.org/abs/0907.4822
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Amôres, Eduardo B, Jesus, Ricardo M, Moitinho, André, Arsenijevic, Vladan, Levenhagen, Ronaldo S, Marshall, Douglas J, Kerber, Leandro O, Künzel, Roseli, Moura, Rodrigo A
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Dec2021, Vol. 508 Issue 2, p1788-1797, 10p