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We have identified 139 cool carbon stars in the near-infrared spectro-photometric survey of the InfraRed Telescope in Space (IRTS) from the conspicuous presence of molecular absorption bands at 1.8, 3.1 and 3.8 microns. Among them 14 are…

Astrophysics · Physics 2007-05-23 T. Le Bertre , M. Tanaka , I. Yamamura , H. Murakami , D. J. MacConnell

Infrared imaging properties of dusty winds around late-type stars are investigated in detail, employing a self-consistent model that couples the equations of motion and radiative transfer. Because of general scaling properties, the angular…

Astrophysics · Physics 2015-06-24 Zeljko Ivezic , Moshe Elitzur

We present here the first observation of galactic AGB stars with the InfraRed Array Camera (IRAC) onboard the Spitzer Space Telescope. Our sample consists of 48 AGB stars of different chemical signature, mass loss rate and variability…

Astrophysics · Physics 2009-06-23 Massimo Marengo , Megan Reiter , Giovanni G. Fazio

We present 10 - 19 um moderate resolution spectra of ten M dwarfs, one L dwarf, and two T dwarf systems obtained with the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. The IRS allows us to examine molecular spectroscopic…

This paper presents combined ${\it Spitzer}$ IRAC and ${\it Hubble}$ COS results for a double-blind survey of 195 single and 22 wide binary white dwarfs for infrared excesses and atmospheric metals. The selection criteria include cooling…

Earth and Planetary Astrophysics · Physics 2019-04-24 Thomas G. Wilson , Jay Farihi , Boris T. Gänsicke , Andrew Swan

We present a catalogue of variable stars in the near-infrared wavelength detected with overlapping regions of the 2MASS public images, and discuss their properties. The investigated region is in the direction of the Galactic center (-30 < l…

Solar and Stellar Astrophysics · Physics 2014-11-20 Shinjirou Kouzuma , Hitoshi Yamaoka

We present the results of a near-infrared monitoring programme of a selected sample of stars, initially suspected to be Mira variables and OH/IR stars, covering more than a decade of observations. The objects monitored cover the typical…

Astrophysics · Physics 2016-08-15 F. M. Jiménez-Esteban , P. García-Lario , D. Engels , A. Manchado

Despite having different astronomical characteristics, the studies of mira variables and ultra-cool dwarfs frequently show similar red colors, which could cause leading to photometric misclassification. This study uses photometric data from…

Solar and Stellar Astrophysics · Physics 2024-09-18 Aleksandra Avdeeva , Kefeng Tan , Santosh Joshi , Dana Kovaleva , Harinder P. Singh , Ali Luo , Oleg Malkov

{The selection of AGB C and M stars from NIR colours has been done in recent years using adjustable criteria that are in needs of standardization if one wants to compare, in a coherent manner, properties of various populations.} We intend…

Astrophysics · Physics 2009-11-13 P. Battinelli , S. Demers , F. Mannucci

We present the culmination of our near-infrared survey of the optically spectroscopically identified white dwarf stars from the McCook & Sion catalog, conducted using photometric data from the Two Micron All Sky Survey final All Sky Data…

In this paper we present optical and near-infrared finding charts, accurate astrometry (~1") and single-epoch near-infrared photometry for 371 IRAS sources, 96% of those included in the so-called Arecibo sample of OH/IR stars (Eder et al.…

Astrophysics · Physics 2007-05-23 F. M. Jiménez-Esteban , L. Agudo-Mérida , D. Engels , P. García-Lario

In this paper we present a catalog which includes 141 bright candidates ($\leq10.27$ mag, V band) showing the infrared (IR) excess at 22 $\mu$m. Of which, 38 stars are known IR excess stars or disk, 23 stars are double or multiple stars and…

Solar and Stellar Astrophysics · Physics 2013-10-10 Chao-Jian Wu , Hong Wu , Man-I Lam , Ming Yang , Xiao-Qing Wen , Shuo Li , Tong-Jie Zhang , Liang Gao

The dynamical structure and infrared emission of winds around late-type stars are studied in a self-consistent model that couples the equations of motion and radiative transfer. Both the dynamics and IR spectrum of the solution are fully…

Astrophysics · Physics 2016-08-30 Zeljko Ivezic , Moshe Elitzur

We report the spectroscopic and photometric monitoring of a sample of 530 candidate AGB stars in a 5 degrees field, selected from the IPHAS catalog: historic light curves were derived from Asiago IR plates taken in the years 1965 -1984. We…

Solar and Stellar Astrophysics · Physics 2018-05-24 Roberto Nesci , Taavi Tuvikene , Corinne Rossi , Silvia Gaudenzi , Silvia Galleti , Paolo Ochner , Harry Enke , .

We report the discovery of 87 new T dwarfs uncovered with the Wide-field Infrared Survey Explorer (WISE) and three brown dwarfs with extremely red near-infrared colors that exhibit characteristics of both L and T dwarfs. Two of the new T…

We present the Spitzer Atlas of Stellar Spectra (SASS), which includes 159 stellar spectra (5 to 32 mic; R~100) taken with the Infrared Spectrograph on the Spitzer Space Telescope. This Atlas gathers representative spectra of a broad…

We present the discovery of a source with broadband infrared photometric characteristics similar to Sakurai's Object. WISE J180956.27-330500.2 (hereafter, J1810-3305) shows very red WISE colors, but a very blue 2MASS [K] vs. WISE [W1 (3.4…

Solar and Stellar Astrophysics · Physics 2015-06-04 Poshak Gandhi , Issei Yamamura , Satoshi Takita

We discuss optical and infrared photometric properties of stars matched in the Two Micron All Sky Survey (2MASS) and the Sloan Digital Sky Survey (SDSS) commissioning data for 50 deg2 of sky. About 98% (63,000) of objects listed in the…

Astrophysics · Physics 2008-11-26 K. Finlator , Z. Ivezic , M. Strauss , J. Knapp , R. Lupton , J. Gunn , C. Rockosi

We find that AGB stars separate in the 25-12 vs. 12-K color-color diagram according to their chemistry (O, S vs. C) and variability type (Miras vs. SRb/Lb). While discrimination according to the chemical composition is not surprising, the…

Astrophysics · Physics 2007-05-23 Zeljko Ivezic , Gillian R. Knapp

Known bright S stars, recognized as such by their enhanced s-process abundances and C/O ratio, are typically members of the asymptotic giant branch (AGB) or the red giant branch (RGB). Few modern digital spectra for these objects have been…

Solar and Stellar Astrophysics · Physics 2015-05-28 Elizabeth Otto , Paul J Green , Richard O. Gray