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We present high signal to noise ratio Spitzer Infrared Spectrograph observations of 17 Virgo early-type galaxies. The galaxies were selected from those that define the colour-magnitude relation of the cluster, with the aim of detecting the…

We present Spitzer Space Telescope observations of the well-studied extremely red objects (EROs) HR10 and LBDS53W091 from 3.6 to 160 microns. These galaxies are the prototypes of the two primary classes of EROs: dusty starbursts and old,…

Astrophysics · Physics 2010-11-11 Daniel Stern , Ranga-Ram Chary , Peter Eisenhardt , Leonidas Moustakas

The nebula J222557+601148, tentatively identified by Morris et al. (2006) as a young Galactic supernova remnant (SNR) from Spitzer Galactic First Look Survey images and a follow-up mid-infrared spectrum, is unlikely to be a SNR remnant…

Solar and Stellar Astrophysics · Physics 2015-05-18 Robert Fesen , Dan Milisavljevic

The 6.67 hr periodicity and the variable X-ray flux of the central compact object (CCO) at the center of the SNR RCW 103, named 1E 161348-5055, have been always difficult to interpret within the standard scenarios of an isolated neutron…

High Energy Astrophysical Phenomena · Physics 2016-09-07 Nanda Rea , Alice Borghese , Paolo Esposito , Francesco Coti Zelati , Matteo Bachetti , Gian Luca Israel , Andrea De Luca

We present a near-infrared (NIR) variability analysis for an 6\arcmin $\times$ 6\arcmin region, which encompasses the massive protocluster G286.21+0.17. The total sample comprises more than 5000 objects, of which 562 show signs of a…

Astrophysics of Galaxies · Physics 2020-07-08 Yu Cheng , Morten Andersen , Jonathan C. Tan

The recent variability survey of the NGC 3766 cluster revealed a considerable number of periodic variable stars in a region of the H-R diagram where no pulsation is expected. This region lies between the instability strips of the delta…

Solar and Stellar Astrophysics · Physics 2014-09-10 S. J. A. J. Salmon , J. Montalbàn , D. R. Reese , M. -A. Dupret , P. Eggenberger

GRB 090709A is a long gamma-ray burst (GRB) discovered by Swift, featuring a bright X-ray afterglow as well as a faint infrared transient with very red and peculiar colors. The burst attracted a large interest because of a possible…

High Energy Astrophysical Phenomena · Physics 2015-05-14 A. De Luca , P. Esposito , G. L. Israel , D. Götz , G. Novara , A. Tiengo , S. Mereghetti

We report on two Chandra observations of the quasar PSO J0309+27, the most distant blazar observed so far (z=6.1), performed eight months apart, in March and November 2020. Previous Swift-XRT observation showed that this object is one of…

Neutron stars can appear as sources of different nature. In this paper we address observability of a hypothetical class of neutron stars -- HOt and Fast Non Accreting Rotators, HOFNARs. These objects are heated due to the r-mode…

High Energy Astrophysical Phenomena · Physics 2023-10-02 A. D. Khokhriakova , A. I. Chugunov , S. B. Popov , M. E. Gusakov , E. M. Kantor

We have observed 13 z >= 4.5 QSOs using the Multiband Imaging Photometer for Spitzer, nine of which were also observed with the Infrared Array Camera. The observations probe rest wavelengths ~ 0.6-4.3 micron, bracketing the local minimum in…

Astrophysics · Physics 2010-11-11 D. C. Hines , O. Krause , G. H. Rieke , X. Fan , M. Blaylock , G. Neugebauer

We present VLT near-IR spectroscopic observations of three X-ray sources characterized by extremely high X-ray-to-optical ratios (X/O>40), extremely red colors (6.3<R-K<7.4, i.e. EROs) and bright infrared magnitudes (17.6<K<18.3). These…

We report the discovery of a large number of short-period variable stars in the dwarf irregular galaxy NGC6822, based on deep time-series imaging carried out with the ESO Very Large Telescope. In particular, we found a modest population of…

Astrophysics · Physics 2009-11-07 G. Clementini , E. V. Held , L. Baldacci , L. Rizzi

We present the results of a photometric study of RR Lyrae variables in the field of the globular cluster M55. We have discovered nine new RR Lyrae stars, increasing the number of known variables in this cluster to 15 objects. Five of the…

Astrophysics · Physics 2009-10-31 A. Olech , J. Kaluzny , I. B. Thompson , W. Pych , W. Krzeminski , A. Schwarzenberg-Czerny

We obtained optical spectra of four objects identified with variable radio sources. Three objects (0029+0554, 0400+0550, 2245+0500) were found to be quasars with redshifts of 1.314, 0.761, and 1.091. One object (2349+0534) has a continuum…

Astrophysics · Physics 2009-11-07 V. Chavushyan , R. Mujica , A. G. Gorshkov , V. K. Konnikova , M. G. Mingaliev

"Little red dots" (LRDs) represent a new population of astronomical objects uncovered by JWST whose nature remains debated. Although many LRDs are suspected as active galactic nuclei (AGN), they show little variability on days-years…

This paper presents the Charge-Coupled Device time-series photometric observations of the open cluster NGC 1582 and its surrounding field with Johnson B, V and R filters by using Nanshan 1m telescope of Xinjiang Astronomical Observatory. 19…

Solar and Stellar Astrophysics · Physics 2018-09-27 Fang-Fang Song , Ali Esamdin , Lu Ma , Jin-Zhong Liu , Yu Zhang , Hu-Biao Niu , Tao-Zhi Yang

We present a new X-ray selected high redshift quasar CXOCY J125304.0-090737 at z=4.179, discovered by the Calan-Yale Deep Extragalactic Research (CYDER) Survey. This quasar is the fifth X-ray selected high redshift radio quiet quasar…

Astrophysics · Physics 2009-11-07 F. J. Castander , E. Treister , T. J. Maccarone , P. S. Coppi , J. Maza , S. E. Zepf , R. Guzman

According to the Hubble law, high redshift objects such as Quasar (QSOs), X-ray Active Galactic Nuclei (AGN) together with the Gamma Ray Burst (GRBs) are the fastest and farthest objects. These characteristics provides strong motivations…

Astrophysics · Physics 2008-07-04 C. E. Navia , C. R. A. Augusto , K. H. Tsui

We present the results of high-resolution (1-0.4A) optical spectroscopy of a sample of very low-mass stars. These data are used to examine the kinematics of the stars at the bottom of the hydrogen-burning main sequence. No evidence is found…

Astrophysics · Physics 2009-10-30 C. G. Tinney , I. N. Reid

One of the first massive stars detected in X-rays, Schulte 12 has remained a puzzle in several aspects. In particular, its extreme brightness both in the visible and X-ray ranges is intriguing. Thanks to Swift and XMM-Newton observations…

Solar and Stellar Astrophysics · Physics 2020-12-09 Yael Naze , Gregor Rauw , Stefan Czesla , Laurent Mahy , Fran Campos